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LUND UNIVERSITY
PO Box 117221 00 Lund+46 46-222 00 00
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar CellApplications “Tiny Crystals for Big Applications”
Qenawy, Mohamed
2015
Link to publication
Citation for published version (APA):Qenawy, M. (2015). Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar CellApplications “Tiny Crystals for Big Applications”. Division of Chemical Physics, Department of Chemistry, LundUniversity.
Total number of authors:1
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Ultrafast Ultrafast Ultrafast Ultrafast Photoinduced Photoinduced Photoinduced Photoinduced ProcessesProcessesProcessesProcesses in in in in Core Core Core Core and and and and CoreCoreCoreCore––––Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots for for for for Solar Cell Solar Cell Solar Cell Solar Cell
ApplicationApplicationApplicationApplicationssss
““““Tiny Tiny Tiny Tiny Crystals Crystals Crystals Crystals for for for for Big ApplicationsBig ApplicationsBig ApplicationsBig Applications””””
Mohamed Mohamed Mohamed Mohamed Ahmed Ahmed Ahmed Ahmed AbdellahAbdellahAbdellahAbdellah
Doctoral Doctoral Doctoral Doctoral DissertationDissertationDissertationDissertation
Faculty opponent
Professor Prashant V. KamatPrashant V. KamatPrashant V. KamatPrashant V. Kamat, Professor of Science
Radiation Laboratory and Department of Chemical & Bimolecular Engineering,
University of Notre Dame, Indiana, United States
Organization: Lund University,: Lund University,: Lund University,: Lund University, Chemistry Department,Chemistry Department,Chemistry Department,Chemistry Department, Division of Chemical Physics, P.O. Box 124 SEDivision of Chemical Physics, P.O. Box 124 SEDivision of Chemical Physics, P.O. Box 124 SEDivision of Chemical Physics, P.O. Box 124 SE----221 00, 221 00, 221 00, 221 00, Lund, SwedenLund, SwedenLund, SwedenLund, Sweden
Document name: Doctoral Dissertation: Doctoral Dissertation: Doctoral Dissertation: Doctoral Dissertation
Date of issue: 2015: 2015: 2015: 2015----02020202----16161616
Author: : : : Mohamed Ahmed AbdellahMohamed Ahmed AbdellahMohamed Ahmed AbdellahMohamed Ahmed Abdellah QenawyQenawyQenawyQenawy
Title: Ultrafast Ultrafast Ultrafast Ultrafast Photoinduced Photoinduced Photoinduced Photoinduced ProcessesProcessesProcessesProcesses in in in in Core Core Core Core and and and and CoreCoreCoreCore––––Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots for for for for Solar Cell ApplicationSolar Cell ApplicationSolar Cell ApplicationSolar Cell Applicationssss
““““Tiny Tiny Tiny Tiny Crystals Crystals Crystals Crystals for for for for Big ApplicationsBig ApplicationsBig ApplicationsBig Applications””””
Abstract The balance between our demands of energy and the energy we are consuming is not in equilibrium anymore. Therefore, the search for other energy resources is indispensable. Sustainable energy sources offer the alternative to the fossil fuels. Within many types of sustainable energy sources, solar energy offers more than the total global energy consumption. Solar cells are the smart conversion tools to harvest the incident photons and create electricity out of these photons. Solar cells have passed through different generations where two important factors control the solar cells market. The solar cell efficiency and price play the cornerstones in the solar cell marketing. Third generation of solar cells aims to maximize the price–performance equation by using cheap materials without compromising efficiency. Nanomaterials have emerged as the promising building blocks to harvest the solar light in the third generation of the solar cells. Among them, quantum dots (QDs) can be used as viable candidate due to their superb features such as high extinction coefficient, a tunable absorption edge, and the possibility to generate and collect multiple excitons by using single, high energy photon. Both the behaviors of photoexcited electrons and holes determine the overall efficiency of QD based solar cells. This thesis presents a systematic study of the ultrafast photoinduced charge dynamics in QD solar cell materials including the charge transfer, exciton migration, carrier trapping and their influence on real solar cell performance. The materials investigated start with conventional neat core CdSe QDs and extend to gradient Cd1-xSe1-yZnxSy core–shell (CS) QDs. The latter are used to obtain improved optical and device performance. The electron injection from CdSe into ZnO nanowires were first observed to be very fast (few ps). This fast electron injection encourages us to study the possibility to inject multiple electrons from a QD under high excitation conditions. We revealed that a competition between electron injection and Auger recombination occurs.
Compared with electrons, the photoinduced holes are more likely to be trapped. However, such trap states sometimes can be radiative with long lifetime up to tens of microseconds in oleic acid capped CdSe QDs. In this scenario, the hole injection in p-type QD solar cells are proved to be less efficient (<10%) compared with electron injection in n-type counterparts. It is highly affected by the surface trapping sites induced by the linker exchange process. The hole injection can then be improved by passivating the surface trap sites using core shell structures. Besides electron or hole injection, exciton migration can also occur via Förster resonant energy transfer (FRET). We found that FRET between QDs would enable to make use of the absorption of light by the indirectly attached QDs in QD-sensitized metal oxide (MO) anodes. In well-organized multi-sized QD mixtures, the energy transfer is even more pronounced. We experimentally observed the FRET process in randomly arranged multi-sized QD assembly and tandem stacked QD layers by using time-resolved and steady-state spectroscopies. Theoretical simulations where dipole distribution model was introduced for coupling calculations complies well with the experimental results. In order to minimize the effect of surface defects and improve the photostability of QD solar cells, we investigated the core–shell QD system where the surface trapping of carriers can be well passivated by shell materials with enhanced optical properties and device performance. Herein, a wider band gap semiconductor is employed as a shield shell around the active core in gradient growth, known as gradient Cd1-xSe1-yZnxSy CSQDs. Such QDs offer higher photostability, higher fluorescence quantum yield, and less interfacial defects than the conventional step-like CSQDs. We first characterized the gradient CSQDs using steady-state optical spectroscopy and HR-TEM images in order to determine their dimensions and to evaluate the shell thickness. Then XRD and EDX were used to characterize the chemical composition and the crystal structures.
The photodynamic of these CSQDs in photovoltaic systems was also studied. We first found that the electron injection from the active core to n-type MO showed relatively larger exponential shell thickness dependence compared with step-like CSQDs. We established that the highest electron injection efficiency (~ 80%) can be found with shell thickness up to 1.3 nm. Such shell also allows high surface passivation providing optimal conditions for charge collection in solar cells. Finally, we integrated our knowledge about the electron and hole behaviors to explain the solar cell performances according to the core–shell structure. We confirmed that the hole trapping is the critical factor for QD-sensitized solar cell efficiency. The trapping can be well repaired by using optimal core–shell structure.
Key words: Quantum dots, coreQuantum dots, coreQuantum dots, coreQuantum dots, core––––shell, electron injection, hole injection, hole trapping, exciton migration, solar shell, electron injection, hole injection, hole trapping, exciton migration, solar shell, electron injection, hole injection, hole trapping, exciton migration, solar shell, electron injection, hole injection, hole trapping, exciton migration, solar cells, ultrafast dynamics, timecells, ultrafast dynamics, timecells, ultrafast dynamics, timecells, ultrafast dynamics, time----resolved spectroscopy.resolved spectroscopy.resolved spectroscopy.resolved spectroscopy. Classification system and/or index terms (if any) Language: English: English: English: English
Supplementary bibliographical information ISBN: ISSN and key title Price Recipient’s notes Number of pages: Security classification
I, the undersigned, being the copyright owner of the abstract of the above-mentioned dissertation, hereby grant to all reference sources permission to publish and disseminate the abstract of the above-mentioned dissertation.
Signature: Date: 2015-02-16
Ultrafast Photoinduced Ultrafast Photoinduced Ultrafast Photoinduced Ultrafast Photoinduced ProcessesProcessesProcessesProcesses in in in in Core and CoreCore and CoreCore and CoreCore and Core––––Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots Shell Quantum Dots
for Solar Cell for Solar Cell for Solar Cell for Solar Cell ApplicationApplicationApplicationApplicationssss
“Tiny “Tiny “Tiny “Tiny Crystals Crystals Crystals Crystals for for for for Big ApplicationsBig ApplicationsBig ApplicationsBig Applications””””
Mohamed Mohamed Mohamed Mohamed Ahmed Ahmed Ahmed Ahmed AbdellahAbdellahAbdellahAbdellah
Doctoral DissertationDoctoral DissertationDoctoral DissertationDoctoral Dissertation
Academic thesis, which by due permission of the Faculty of Science, Lund University, will be publicly defended on Friday 13th of March, 2015 at 09:15 a.m. in lecture hall C, at the Center of Chemistry and Chemical Engineering, Getingevägen 60, Lund, for the degree of Doctor of Philosophy in Science.
Cover picture: Quantum dots for solar energy harvesting by Maiy A. ElQuantum dots for solar energy harvesting by Maiy A. ElQuantum dots for solar energy harvesting by Maiy A. ElQuantum dots for solar energy harvesting by Maiy A. El----wakeelwakeelwakeelwakeel....
Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah
Full name: Mohamed Ahmed Abdellah QenawyMohamed Ahmed Abdellah QenawyMohamed Ahmed Abdellah QenawyMohamed Ahmed Abdellah Qenawy
Copyright © Mohamed Abdellah© Mohamed Abdellah© Mohamed Abdellah© Mohamed Abdellah
Department of Chemical Physics, Faculty of Science, Lund University, Sweden
ISBN 978978978978----91919191----7422742274227422----388388388388----0000 Printed in Sweden by Media-Tryck, Lund University Lund 2015
5اآليه سورة الضحى “And your Lord (ALLAH) is going to give you (Prophet Muhammed), and you will be satisfied” Surat Al-Duhaa 5
Dedicated to,
Soul of my mother
Soul of my father-in-law
Dalia
Eyad, Yahia and Dareen
Contents
AbstractAbstractAbstractAbstract.......................................................................................................... i AcknowledgementsAcknowledgementsAcknowledgementsAcknowledgements........................................................................................ iii List of papersList of papersList of papersList of papers................................................................................................. vi Contribution reportContribution reportContribution reportContribution report...................................................................................... viii Abbreviations and symbolsAbbreviations and symbolsAbbreviations and symbolsAbbreviations and symbols........................................................................... xi Chapter 1: IntroductionChapter 1: IntroductionChapter 1: IntroductionChapter 1: Introduction............................................................................... 1 1.1 Sustainable energy sources.................................................................... 1 1.2 Quantum Dot (QD)............................................................................ 2 1.3 Quantum Dot (QD) properties........................................................... 4 1.4 Core–shell quantum dots (CSQDs)…………………………………. 5 1.5 Quantum dots applications.................................................................. 6 1.6 Quantum dots toxicity......................................................................... 7 Chapter 2: Experimental methodsChapter 2: Experimental methodsChapter 2: Experimental methodsChapter 2: Experimental methods................................................................ 9 2.1 Materials.............................................................................................. 9 2.2 Synthesis of neat CdSe QDs………………………………………… 9 2.3 Synthesis of gradient Cd1-xZnxSe1-ySy CSQDs…...................………… 10 2.4 QDs surface ligand exchange……………………....………………… 10 2.5 ZnO NWs and NiO mesoporous film preparation……….………….. 11 2.6 QDs characterization………………………………………….……... 11 2.7 Solar cell device fabrication………………………………………….. 12 2.8 Transient absorption spectroscopy (TA)…………………………...… 12 2.9 Time-resolved PL spectroscopy (TRPL)……………………………... 13 2.10 Time-resolved terahertz spectroscopy (THz)……………………….. 14 2.11 X-ray diffraction (XRD)………………………………….………… 14 Chapter 3: Exciton dynamics in QDsChapter 3: Exciton dynamics in QDsChapter 3: Exciton dynamics in QDsChapter 3: Exciton dynamics in QDs…………………………….………. 15 3.1 Motivation…………………………………………………………... 15 3.2 Steady-state absorption and emission…………………….………….. 15 3.3: Exciton dynamics…………………………………………………… 17 3.4 Paper I “Electron injection from QDs to MO”……………………… 20 3.5 Paper II “Multiple exciton harvesting”………………………………. 22 3.6 Paper III “Ultra-long-lived trapped holes in QDs”…………………... 25 3.7 Paper IV “Hole injection vs hole trapping”………………………….. 27 3.8 Paper V “Energy transfer in CdSe-ZnO NWs system”………………. 30 3.9 Paper VI “Energy funneling through multi-sized QD films”………... 33
Chapter 4: Photoinduced dynamics in coreChapter 4: Photoinduced dynamics in coreChapter 4: Photoinduced dynamics in coreChapter 4: Photoinduced dynamics in core––––shell QDsshell QDsshell QDsshell QDs………………...... 37 4.1 Motivation…………………………………………………………... 37 4.2 Classification of core–shell QDs……………………………………... 37 4.3 Important aspects for preparing the gradient type I
CSQDs……………………………………………..………….……. 39
4.4 Characterization of type I gradient Cd1-xZnxSe1-ySy CSQDs………..… 41 4.5 Paper VII “Electron injection from gradient Cd1-xZnxSe1-ySy CSQDs to
MO”…………………………………………………………….…... 45
4.6 Paper VIII “hole trapping vs quantum dot sensitized solar cell performance”……………………………….………………………...
48
Chapter 5: Conclusions and future workChapter 5: Conclusions and future workChapter 5: Conclusions and future workChapter 5: Conclusions and future work………………………..………... 51 Svensk sammanfattningSvensk sammanfattningSvensk sammanfattningSvensk sammanfattning……………………………………………………. 54
Arabic summary (Arabic summary (Arabic summary (Arabic summary (الملخص العربىالملخص العربىالملخص العربىالملخص العربى))))………………………………….….……… 57
References….References….References….References….……………………………………………………..………... 60
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
i
Abstract
The balance between our demands of energy and the energy we are consuming is not
in equilibrium anymore. Therefore, the search for other energy resources is
indispensable. Sustainable energy sources offer the alternative to the fossil fuels. Within
many types of sustainable energy sources, solar energy offers more than the total global
energy consumption. Solar cells are the smart conversion tools to harvest the incident
photons and create electricity out of these photons. Solar cells have passed through
different generations where two important factors control the solar cells market. The
solar cell efficiency and price play the cornerstones in the solar cell marketing. Third
generation of solar cells aims to maximize the price–performance equation by using
cheap materials without compromising efficiency. Nanomaterials have emerged as the
promising building blocks to harvest the solar light in the third generation of the solar
cells. Among them, quantum dots (QDs) can be used as viable candidate due to their
superb features such as high extinction coefficient, a tunable absorption edge, and the
possibility to generate and collect multiple excitons by using single, high energy
photon. Both the behaviors of photoexcited electrons and holes determine the overall
efficiency of QD based solar cells. This thesis presents a systematic study of the ultrafast
photoinduced charge dynamics in QD solar cell materials including the charge transfer,
exciton migration, carrier trapping and their influence on real solar cell performance.
The materials investigated start with conventional neat core CdSe QDs and extend to
gradient Cd1-xSe1-yZnxSy core–shell (CS) QDs. The latter are used to obtain improved
optical and device performance. The electron injection from CdSe into ZnO nanowires
were first observed to be very fast (few ps). This fast electron injection encourages us to
study the possibility to inject multiple electrons from a QD under high excitation
conditions. We revealed that a competition between electron injection and Auger
recombination occurs.
Compared with electrons, the photoinduced holes are more likely to be trapped.
However, such trap states sometimes can be radiative with long lifetime up to tens of
microseconds in oleic acid capped CdSe QDs. In this scenario, the hole injection in p-
type QD solar cells are proved to be less efficient (<10%) compared with electron
injection in n-type counterparts. It is highly affected by the surface trapping sites
induced by the linker exchange process. The hole injection can then be improved by
passivating the surface trap sites using core shell structures. Besides electron or hole
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
ii
injection, exciton migration can also occur via Förster resonant energy transfer (FRET).
We found that FRET between QDs would enable to make use of the absorption of
light by the indirectly attached QDs in QD-sensitized metal oxide (MO) anodes. In
well-organized multi-sized QD mixtures, the energy transfer is even more pronounced.
We experimentally observed the FRET process in randomly arranged multi-sized QD
assembly and tandem stacked QD layers by using time-resolved and steady-state
spectroscopies. Theoretical simulations where dipole distribution model was
introduced for coupling calculations complies well with the experimental results. In
order to minimize the effect of surface defects and improve the photostability of QD
solar cells, we investigated the core–shell QD system where the surface trapping of
carriers can be well passivated by shell materials with enhanced optical properties and
device performance. Herein, a wider band gap semiconductor is employed as a shield
shell around the active core in gradient growth, known as gradient Cd1-xSe1-yZnxSy
CSQDs. Such QDs offer higher photostability, higher fluorescence quantum yield, and
less interfacial defects than the conventional step-like CSQDs. We first characterized
the gradient CSQDs using steady-state optical spectroscopy and HR-TEM images in
order to determine their dimensions and to evaluate the shell thickness. Then XRD
and EDX were used to characterize the chemical composition and the crystal structures.
The photodynamic of these CSQDs in photovoltaic systems was also studied. We
first found that the electron injection from the active core to n-type MO showed
relatively larger exponential shell thickness dependence compared with step-like
CSQDs. We established that the highest electron injection efficiency (~ 80%) can be
found with shell thickness up to 1.3 nm. Such shell also allows high surface passivation
providing optimal conditions for charge collection in solar cells. Finally, we integrated
our knowledge about the electron and hole behaviors to explain the solar cell
performances according to the core–shell structure. We confirmed that the hole
trapping is the critical factor for QD-sensitized solar cell efficiency. The trapping can
be well repaired by using optimal core–shell structure.
Acknowledgements
iii
Acknowledgements
‘‘A person who is not thankful to his benefactor is not thankful to ALLAHA person who is not thankful to his benefactor is not thankful to ALLAHA person who is not thankful to his benefactor is not thankful to ALLAHA person who is not thankful to his benefactor is not thankful to ALLAH’’, Prophet MuhammedProphet MuhammedProphet MuhammedProphet Muhammed
First of all, praise is to ALLAHALLAHALLAHALLAH, the most Merciful for his gifts.
Second of all, I would like to apologize in advance if somehow I forgot to express my
gratitude to any one that gave a hand in order to make this work real. Anyway, I will
try to do my best to give everyone his right in the acknowledgment. Since 29th of
November 2010, I started as a PhD student in Chemical Physics department. That was
my dream once I arrived to Sweden therefore I would like to express my sincere
gratitude to these fantastic people. In particular to:
My main supervisor Prof. Tõnu PulleritsTõnu PulleritsTõnu PulleritsTõnu Pullerits first for accepting me as a guest PhD then
for the opportunity he gave me to continue my PhD studies in Chemical Physics
department, for introducing me to the quantum dots in solar cell application project,
for his continuous and innumerable help, support, discussion, science and
encouragement. Honestly if I will talk about TõnuTõnuTõnuTõnu, I think I need more than one thesis
to express how he was helpful and supportive in everything. The head of the
department Prof. Villy SundströmVilly SundströmVilly SundströmVilly Sundström for giving me the chance to continue my PhD
studies in this amazing research environment.
My co-supervisors, Dr. Karel ŽídekKarel ŽídekKarel ŽídekKarel Žídek (Dearest boss) and Dr. Kaibo Zheng Kaibo Zheng Kaibo Zheng Kaibo Zheng
(Kaiboscopy, Kaiboskite, etc). Actually I do not know what to say about these smart
guys. I want to say without you this work will stay in dark. To have a nice friend that
is awesome. To have a nice co-supervisor that is luck. For me I had both in one. KaiboKaiboKaiboKaibo
and KarelKarelKarelKarel you taught me a lot and if I think how to pay back, no letters or words or
sentences, are enough to pay back your help and support. Dr. Khadga J. KarkiKhadga J. KarkiKhadga J. KarkiKhadga J. Karki thanks
a lot for all the nice work we had together in Lund or in (Oregon) USA and for useful
and interesting discussion.
Chemical Physics amazing leaders, ArkadyArkadyArkadyArkady, IvanIvanIvanIvan, DonatasDonatasDonatasDonatas, TorbjörnTorbjörnTorbjörnTorbjörn and EbbeEbbeEbbeEbbe
thanks for all the time we discuss about science or life related issues. It was a great time
to play football, tennis table, floor ball, ice skiing, and ice skating. Pullerits’s Pullerits’s Pullerits’s Pullerits’s group
current and former members, AtsunoriAtsunoriAtsunoriAtsunori, Junshen Junshen Junshen Junshen (brother), Nils Nils Nils Nils (nilspedia), EvaEvaEvaEva,
SeshaSeshaSeshaSesha, FadiFadiFadiFadi, ThorstenThorstenThorstenThorsten, RebeccaRebeccaRebeccaRebecca, MehrnazMehrnazMehrnazMehrnaz, SumeraSumeraSumeraSumera, MadhuriMadhuriMadhuriMadhuri, Abdelrazik MousaAbdelrazik MousaAbdelrazik MousaAbdelrazik Mousa,
and Abdallah AbdelwahabAbdallah AbdelwahabAbdallah AbdelwahabAbdallah Abdelwahab I could not have done this work without the former
members experience and the current members collaboration. Therefore, thanks a lot.
Acknowledgements
iv
Chemical Physics department current and former members, AliceAliceAliceAlice (tobeb), AbomaAbomaAbomaAboma
(Obama), ErikErikErikErik, AmalAmalAmalAmal (Reeeeta), AhmedAhmedAhmedAhmed, TobiasTobiasTobiasTobias, KasperKasperKasperKasper, MainakMainakMainakMainak, DavidDavidDavidDavid, CarlitoCarlitoCarlitoCarlito,
AhiburAhiburAhiburAhibur, ErlingErlingErlingErling, YuxiYuxiYuxiYuxi, DanielaDanielaDanielaDaniela, JensJensJensJens, WeiWeiWeiWei, TomasTomasTomasTomas, MartinMartinMartinMartin, MatthiasMatthiasMatthiasMatthias, DimaliDimaliDimaliDimali,
KamalKamalKamalKamal, SamirSamirSamirSamir, RafaelRafaelRafaelRafael, JakubJakubJakubJakub, LottaLottaLottaLotta, KarinKarinKarinKarin, HelenaHelenaHelenaHelena, YingyotYingyotYingyotYingyot, and SunnySunnySunnySunny thanks for
the nice and funny time we had in the lab to break the daily boring routine.
Our department unknown soldiers Maria LevinMaria LevinMaria LevinMaria Levin, Thomas BjorkmanThomas BjorkmanThomas BjorkmanThomas Bjorkman, AnnAnnAnnAnn----ChristinChristinChristinChristin
(Anki), and Katarina FredrikssonKatarina FredrikssonKatarina FredrikssonKatarina Fredriksson. I cannot imagine my work without you, you were
always efficient and helpful. Thank you very much. Incoherent football team members
in Victoriastadion, RafaelRafaelRafaelRafael, DonatasDonatasDonatasDonatas, AbomaAbomaAbomaAboma, MatthiasMatthiasMatthiasMatthias, MartinMartinMartinMartin, and GiulianoGiulianoGiulianoGiuliano. Even
thought, we did not win the tournament but we had very nice games. Thank you guys
for such a nice time. Weekly floor ball game members, AbomaAbomaAbomaAboma, PavelPavelPavelPavel, KarelKarelKarelKarel, TomasTomasTomasTomas,
DavidDavidDavidDavid, MartinMartinMartinMartin, ArkadyArkadyArkadyArkady, TorbjörnTorbjörnTorbjörnTorbjörn, EbbeEbbeEbbeEbbe, FadiFadiFadiFadi, and AddisAddisAddisAddis. I know we all suffer from
AbomaAbomaAbomaAboma’s playing style but I think we all enjoyed it. Thanks. My fantastic officemate.
PavelPavelPavelPavel, you are amazing officemate. I was lucky to share you the office during my PhD
studies. Thanks a lot for all the time we spent discussing or talking about science or
other stuff. To RamiRamiRamiRami for revising the Arabic summery. Thanks. GunillaGunillaGunillaGunilla, thank you
very much for your help and efforts during printing my thesis.
To our collaborators at Lund University, Dr. Maria E. MissingMaria E. MissingMaria E. MissingMaria E. Missing and Prof. Reine Reine Reine Reine
WallenbergWallenbergWallenbergWallenberg for HR-TEM images for our QDs. Without your clear images I would
not have been able to do the science I did. To our collaborators at Max-Lab, Dr. Qiushi Qiushi Qiushi Qiushi
ZhuZhuZhuZhu and Dr. Sophie CantonSophie CantonSophie CantonSophie Canton. Really I do not know what to say in order to thank you.
For the long measurements here in Lund Synchrotron or in Argonne National Lab in
USA. Therefore, as long as the time we spent together I thank both of you. QiushiQiushiQiushiQiushi,
you are super nice and you know the way to push me very kindly for more samples.
SophieSophieSophieSophie, please keep watermelon for me for the next beam time. Thanks a lot. To our
collaborators at Technical University of Denmark, Nan ZhuNan ZhuNan ZhuNan Zhu and Prof. Qijin ChiQijin ChiQijin ChiQijin Chi for
the AFM measurements. Thanks for your time and your efforts.
Egyptian Friends in Lund and Uppsala, Ahmed MostafaAhmed MostafaAhmed MostafaAhmed Mostafa, Ahmed FawzyAhmed FawzyAhmed FawzyAhmed Fawzy, Haitham Haitham Haitham Haitham
ElElElEl----taliawytaliawytaliawytaliawy, Wael AwadWael AwadWael AwadWael Awad, Tarek SelimTarek SelimTarek SelimTarek Selim, Abdallah ShokryAbdallah ShokryAbdallah ShokryAbdallah Shokry, Mohamed EssamMohamed EssamMohamed EssamMohamed Essam,
Mohamed MabroukMohamed MabroukMohamed MabroukMohamed Mabrouk, Ibrahim AbdelwahabIbrahim AbdelwahabIbrahim AbdelwahabIbrahim Abdelwahab, Mostafa Mostafa Mostafa Mostafa FekryFekryFekryFekry, Tarik DishishaTarik DishishaTarik DishishaTarik Dishisha,
AbdulrahmanAbdulrahmanAbdulrahmanAbdulrahman, Wael MobarkWael MobarkWael MobarkWael Mobark, Dr. Mohamed IbrahimMohamed IbrahimMohamed IbrahimMohamed Ibrahim, Mohamed IsmailMohamed IsmailMohamed IsmailMohamed Ismail, Yasser Yasser Yasser Yasser
GaberGaberGaberGaber, Mahmoud SayedMahmoud SayedMahmoud SayedMahmoud Sayed, Mohamed HagresMohamed HagresMohamed HagresMohamed Hagres, Mohamed RedaMohamed RedaMohamed RedaMohamed Reda, Nagwa ElnwishyNagwa ElnwishyNagwa ElnwishyNagwa Elnwishy
and Ahmed Elzohry.Ahmed Elzohry.Ahmed Elzohry.Ahmed Elzohry. Good feeling to have friends that bring home to you abroad
therefore, thank you very much guys for the time we spent together playing football,
eating, indoor cooking, and outdoor barbecue.
Acknowledgements
v
My former supervisors in Egypt, Prof. Hasan SalmanHasan SalmanHasan SalmanHasan Salman, and Dr. Mahmmoud SayedMahmmoud SayedMahmmoud SayedMahmmoud Sayed
Chemistry and Physics Departments, respectively at Qena Faculty of Science, South
Valley University, Egypt for their continuous encouragement during my PhD studies
in Sweden. Thank you very much. My colleagues at the Chemistry Department at
Qena Heba NassarHeba NassarHeba NassarHeba Nassar, Hisham ElsoghierHisham ElsoghierHisham ElsoghierHisham Elsoghier, Haytham FawzyHaytham FawzyHaytham FawzyHaytham Fawzy, Ahmed EissaAhmed EissaAhmed EissaAhmed Eissa, and Nada Nada Nada Nada
NabilNabilNabilNabil, for keeping the teaching responsibilities running in our department at Qena
during my study. All the best for you guys.
The funding agencies, the Knut and Alice Wallenberg FoundationKnut and Alice Wallenberg FoundationKnut and Alice Wallenberg FoundationKnut and Alice Wallenberg Foundation, the Swedish Swedish Swedish Swedish
Energy AgencyEnergy AgencyEnergy AgencyEnergy Agency, the Swedish Research CouncilSwedish Research CouncilSwedish Research CouncilSwedish Research Council, and Ministry Ministry Ministry Ministry of Higher Education of Higher Education of Higher Education of Higher Education
and Scientific Research Egypt and Erasmusand Scientific Research Egypt and Erasmusand Scientific Research Egypt and Erasmusand Scientific Research Egypt and Erasmus (FFEEBB program). Thanks a lot for
funding our work.
The souls of my Mother Safaa AbdelrehimSafaa AbdelrehimSafaa AbdelrehimSafaa Abdelrehim, my father-in-law Dr. Mohamed TalaatMohamed TalaatMohamed TalaatMohamed Talaat,
my Master supervisor Dr. Yossif EbeadYossif EbeadYossif EbeadYossif Ebead, my colleagues Prof. NasrNasrNasrNasr MansourMansourMansourMansour and Dr.
Ayman KhalafAyman KhalafAyman KhalafAyman Khalaf, and my student Aya TarekAya TarekAya TarekAya Tarek. All of them except my father-in-law passed
away during my study. I am dedicating this work for all of you and I hope ALLAHALLAHALLAHALLAH,
the Almighty, bless all of you.
Last but definitely not least, to DaliaDaliaDaliaDalia, my wife, really there are no words in any
dictionary could explain how much I should be thankful for you. But if I said that she
took care of my active three kids during my PhD studies, you can imagine how much
I should be thankful. To my mother-in-law Dr. HHHHanan Elmaghrabyanan Elmaghrabyanan Elmaghrabyanan Elmaghraby, just to let you
know you are like my mom. Thanks a lot for taking care of DaliaDaliaDaliaDalia and the kids as well
and for your continuous sincere prayers for me. To Ahmed TalaatAhmed TalaatAhmed TalaatAhmed Talaat, thank you very
much and all the best. EaydEaydEaydEayd, YahiaYahiaYahiaYahia, and DareenDareenDareenDareen, sorry guys to be away from you
during my PhD studies. Please forgive me. Thanks for the time we spent together
during my vacation. You may not understand me now but EyadEyadEyadEyad, I know you love
chemistry, go ahead please. YahiaYahiaYahiaYahia, I know you love laser and I hope you can be better
than me. DareenDareenDareenDareen, my queen, be a way from both chemistry and Laser and focus on
what you like. Thanks guys. To my father Ahmed AbdellahAhmed AbdellahAhmed AbdellahAhmed Abdellah, brother MahmoudMahmoudMahmoudMahmoud, and
sisters ShymaaShymaaShymaaShymaa and EsraaEsraaEsraaEsraa, thanks a lot. To the rest of my family thanks a lot.
Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah Lund 2015Lund 2015Lund 2015Lund 2015
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
vi
List of Papers
This thesis is based on the following pThis thesis is based on the following pThis thesis is based on the following pThis thesis is based on the following papersapersapersapers::::
I. Karel Žídek, Kaibo Zheng, Carlito S. Ponseca, Jr., Maria E. Messing, Reine Wallenberg, Pavel Chábera, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Villy Sundström, and Tõnu Pullerits
“Electron Transfer in QuantumElectron Transfer in QuantumElectron Transfer in QuantumElectron Transfer in Quantum----DotDotDotDot----Sensitized ZnO Nanowires: Sensitized ZnO Nanowires: Sensitized ZnO Nanowires: Sensitized ZnO Nanowires: Ultrafast TimeUltrafast TimeUltrafast TimeUltrafast Time----Resolved Absorption and Terahertz StudyResolved Absorption and Terahertz StudyResolved Absorption and Terahertz StudyResolved Absorption and Terahertz Study”
Journal of American Chemical Society, 134, (2012201220122012), 12110−12117.
II. Karel Žídek, Kaibo Zheng, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Nils Lenngren, Pavel Chábera, and Tõnu Pullerits
“Ultrafast Dynamics of Multiple Exciton Harvesting in the Ultrafast Dynamics of Multiple Exciton Harvesting in the Ultrafast Dynamics of Multiple Exciton Harvesting in the Ultrafast Dynamics of Multiple Exciton Harvesting in the CdSeCdSeCdSeCdSe−ZnO System: Electron Injection −ZnO System: Electron Injection −ZnO System: Electron Injection −ZnO System: Electron Injection versusversusversusversus Auger RecombinationAuger RecombinationAuger RecombinationAuger Recombination”
Nano Letters, 12, (2012201220122012), 6393−6399.
III. Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah****, Khadga J. Karki*, Nils Lenngren, Kaibo Zheng, Torbjörn Pascher, Arkady Yartsev, and Tõnu Pullerits
*Contributed equally to this work
“Ultra Ultra Ultra Ultra LongLongLongLong----Lived Radiative Trap States in CdSe Quantum DotsLived Radiative Trap States in CdSe Quantum DotsLived Radiative Trap States in CdSe Quantum DotsLived Radiative Trap States in CdSe Quantum Dots”
Journal of Physical Chemistry C, 118, (2014201420142014), 21682−21686.
IV. Kaibo Zheng*, Karel Žídek*, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah****, Wei Zhang, Pavel Chábera, Nils Lenngren, Arkady Yartsev, and Tõnu Pullerits
*Contributed equally to this work
“Ultrafast Ultrafast Ultrafast Ultrafast Charge Transfer Charge Transfer Charge Transfer Charge Transfer from CdSe from CdSe from CdSe from CdSe Quantum Dots Quantum Dots Quantum Dots Quantum Dots to pto pto pto p----Type Type Type Type NiO: NiO: NiO: NiO: Hole Injection Hole Injection Hole Injection Hole Injection vs.vs.vs.vs. Hole TrappingHole TrappingHole TrappingHole Trapping”
Journal of Physical Chemistry C, 118, (2014201420142014), 18462−18471.
V. Kaibo Zheng, Karel Žídek, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Magne Torbjörnsson, Pavel Chábera, Shuyan Shao, Fengling Zhang, and Tõnu Pullerits
“Fast Monolayer Adsorption and Slow Energy Transfer in CdSe Fast Monolayer Adsorption and Slow Energy Transfer in CdSe Fast Monolayer Adsorption and Slow Energy Transfer in CdSe Fast Monolayer Adsorption and Slow Energy Transfer in CdSe Quantum Dot Sensitized ZnO NanowiresQuantum Dot Sensitized ZnO NanowiresQuantum Dot Sensitized ZnO NanowiresQuantum Dot Sensitized ZnO Nanowires”
Journal of Physical Chemistry A, 117, (2013201320132013), 5919−5925.
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
vii
VI. Kaibo Zheng, Karel Žídek, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Nan Zhu, Pavel Chábera, Nils Lenngren, Qijin Chi, and Tõnu Pullerits
“Directed Energy Transfer in Films of CdSe Quantum Dots: Beyond Directed Energy Transfer in Films of CdSe Quantum Dots: Beyond Directed Energy Transfer in Films of CdSe Quantum Dots: Beyond Directed Energy Transfer in Films of CdSe Quantum Dots: Beyond the Point Dipole Approximationthe Point Dipole Approximationthe Point Dipole Approximationthe Point Dipole Approximation”
Journal of American Chemical Society, 136, (2014201420142014), 6259−6268.
VII. Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Karel Žídek, Kaibo Zheng, Pavel Chábera, Maria E. Messing, and Tõnu Pullerits
“BalancingBalancingBalancingBalancing Electron Transfer Electron Transfer Electron Transfer Electron Transfer and and and and Surface Passivation Surface Passivation Surface Passivation Surface Passivation inininin Gradient Gradient Gradient Gradient CdSe/ZnS CdSe/ZnS CdSe/ZnS CdSe/ZnS CoreCoreCoreCore----Shell Quantum Dots Attached Shell Quantum Dots Attached Shell Quantum Dots Attached Shell Quantum Dots Attached to ZnOto ZnOto ZnOto ZnO”
Journal of Physical Chemistry Letters, 4, (2013201320132013), 1760−1765.
VIII. Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Rebecca Marschan, Karel Žídek, Maria E. Messing, Abdallah Abdelwahab, Pavel Chábera, Kaibo Zheng, and Tõnu Pullerits
“Hole Trapping: The Critical Factor for Quantum Dot Sensitized Hole Trapping: The Critical Factor for Quantum Dot Sensitized Hole Trapping: The Critical Factor for Quantum Dot Sensitized Hole Trapping: The Critical Factor for Quantum Dot Sensitized Solar Cell PerformanceSolar Cell PerformanceSolar Cell PerformanceSolar Cell Performance”
Journal of Physical Chemistry C, 118, (2014201420142014), 25802−25802.
Reprints were made with permission from the respective publishers.
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
viii
Contribution report
The project was initiated by Prof. Tõnu PulleritsProf. Tõnu PulleritsProf. Tõnu PulleritsProf. Tõnu Pullerits.
Without the fantastic co-authors none of these papers would be
available.
I. Within the team, I prepared and characterized the samples, also I helped
in experimental data collection, and I was involved in the paper writing.
II. Within the team, I prepared and characterized the samples, also I helped
in experimental data collection, and I was involved in the paper writing.
III. With the co-authors, Khadga and I are equally contributing to this work
by designing and preforming the experiments, data analysis and writing
the manuscript. I prepared and characterized the studied samples.
IV. With the co-authors, Kaibo, Karel and I are equally contributing to this
work by designing and preforming the experiments, data analysis and
writing the manuscript. I prepared and characterized the studied samples.
V. With the co-authors, I contributed to this work by preparing and
characterizing the studied samples, also I put hand in the experimental
data analysis and writing the manuscript.
VI. Within the team, I prepared and characterized the samples, also I helped
in experimental data collection, and I was involved in the paper writing.
VII. With the co-authors, I prepared and characterized the samples, I designed
and preformed the experiments, I analyzed the data, and I wrote the first
draft of the manuscript.
VIII. With the co-authors, I prepared and characterized the samples, I designed
and preformed the experiments, I analyzed the data, and I wrote the first
draft of the manuscript.
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
ix
I am a coI am a coI am a coI am a co----author of the following papers which are notauthor of the following papers which are notauthor of the following papers which are notauthor of the following papers which are not included in included in included in included in
this thesisthis thesisthis thesisthis thesis::::
I. Karel Žídek, Kaibo Zheng, Pavel Chábera, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, and Tõnu Pullerits
“Quantum Quantum Quantum Quantum Dot Photodegradation Dot Photodegradation Dot Photodegradation Dot Photodegradation due to CdSedue to CdSedue to CdSedue to CdSe----ZnO ZnO ZnO ZnO Charge Charge Charge Charge TransferTransferTransferTransfer: Transient : Transient : Transient : Transient Absorption StudyAbsorption StudyAbsorption StudyAbsorption Study”
Applied Physics Letters, 100, (2012201220122012), 243111-4.
II. Kaibo Zheng, Karel Žídek, Mohamed Mohamed Mohamed Mohamed AbdellahAbdellahAbdellahAbdellah, Pavel Chábera, Mahmoud S. Abd El-sadek, and Tõnu Pullerits
“Effect of Effect of Effect of Effect of Metal Oxide Morphology Metal Oxide Morphology Metal Oxide Morphology Metal Oxide Morphology on on on on Electron Injection Electron Injection Electron Injection Electron Injection from CdSe from CdSe from CdSe from CdSe Quantum Dots Quantum Dots Quantum Dots Quantum Dots to ZnOto ZnOto ZnOto ZnO”
Applied Physics Letters, 102, (2013201320132013), 163119-5.
III. Khadga J. Karki, Fei Ma, Kaibo Zheng, Karel Žídek, Abdelrazek Mousa, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Maria E. Messing, Reine Wallenberg, Arkady Yartsev, and Tõnu Pullerits
“Multiple Multiple Multiple Multiple Exciton Generation Exciton Generation Exciton Generation Exciton Generation in in in in NanoNanoNanoNano----Crystals RevisitedCrystals RevisitedCrystals RevisitedCrystals Revisited: : : : Consistent Consistent Consistent Consistent Calculation Calculation Calculation Calculation of the of the of the of the Yield Based Yield Based Yield Based Yield Based on on on on PumpPumpPumpPump----Probe Probe Probe Probe SpectroscopySpectroscopySpectroscopySpectroscopy”
Scientific Reports, 3, (2013201320132013), DOI: 10.1038/srep02287.
IV. Nils Lenngren, Tommy Garting, Kaibo Zheng, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Noëlle Lascoux, Fei Ma, Arkady Yartsev, Karel Žídek, and Tõnu Pullerits
“Multiexciton Absorption Cross Sections of CdSe Quantum Dots Multiexciton Absorption Cross Sections of CdSe Quantum Dots Multiexciton Absorption Cross Sections of CdSe Quantum Dots Multiexciton Absorption Cross Sections of CdSe Quantum Dots Determined by Ultrafast SpectrDetermined by Ultrafast SpectrDetermined by Ultrafast SpectrDetermined by Ultrafast Spectroscopyoscopyoscopyoscopy”
Journal of Physical Chemistry Letters, 4, (2013201320132013), 3330–3336.
V. Thorsten Hansen, Karel Žídek, Kaibo Zheng, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Pavel Chábera, Petter Persson, and Tõnu Pullerits
“Orbital Topology Controlling Charge Injection in QuantumOrbital Topology Controlling Charge Injection in QuantumOrbital Topology Controlling Charge Injection in QuantumOrbital Topology Controlling Charge Injection in Quantum----DotDotDotDot----Sensitized Sensitized Sensitized Sensitized Solar CellsSolar CellsSolar CellsSolar Cells”
Journal of Physical Chemistry Letters, 5, (2014201420142014), 1157–1162.
VI. Carlito S. Ponseca, Jr., Tom J. Savenije, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Kaibo Zheng, Arkady Yartsev, Torbjörn Pascher, Tobias Harlang, Pavel Chábera, Tõnu Pullerits, Andrey Stepanov, Jean-Pierre Wolf, and Villy Sundström
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
x
“Organometel Halide Perovskite Solar Cell Materials Rationalized: Organometel Halide Perovskite Solar Cell Materials Rationalized: Organometel Halide Perovskite Solar Cell Materials Rationalized: Organometel Halide Perovskite Solar Cell Materials Rationalized: Ultrafast Charge Generation, High and MicrosecondUltrafast Charge Generation, High and MicrosecondUltrafast Charge Generation, High and MicrosecondUltrafast Charge Generation, High and Microsecond----Long Balanced Long Balanced Long Balanced Long Balanced Mobilities, and Slow RecombinationMobilities, and Slow RecombinationMobilities, and Slow RecombinationMobilities, and Slow Recombination”
Journal of American Chemical Society, 136, (2014201420142014), 5189–5192.
VII. Tom J. Savenije, Carlito S. Ponseca, Lucas Kunneman, Mohamed Mohamed Mohamed Mohamed AbdellahAbdellahAbdellahAbdellah, Kaibo Zheng, Qiushi Zhu, Sophie E. Canton, Ivan G. Scheblykin, Tõnu Pullerits, Arkady Yartsev, and Villy Sundström
“Thermally Activated Exciton Dissociation and Recombination Thermally Activated Exciton Dissociation and Recombination Thermally Activated Exciton Dissociation and Recombination Thermally Activated Exciton Dissociation and Recombination Control theControl theControl theControl the Carrier Dynamics in Organometal Halide PerovskiteCarrier Dynamics in Organometal Halide PerovskiteCarrier Dynamics in Organometal Halide PerovskiteCarrier Dynamics in Organometal Halide Perovskite”
Journal of Physical Chemistry Letters, 5, (2014201420142014), 2189–2194.
VIII. Karel Žídek, Kaibo Zheng, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Pavel Chábera, Tõnu Pullerits, and Masanori Tachyia
“Simultaneous Creation and Recovery of Trap States on Quantum Simultaneous Creation and Recovery of Trap States on Quantum Simultaneous Creation and Recovery of Trap States on Quantum Simultaneous Creation and Recovery of Trap States on Quantum Dots in a Photoirradiated CdSeDots in a Photoirradiated CdSeDots in a Photoirradiated CdSeDots in a Photoirradiated CdSe−ZnO System−ZnO System−ZnO System−ZnO System”
Journal of Physical Chemistry C, 118, (2014201420142014), 27567–27573.
IX. Karel Žídek, Mohamed AbdellahMohamed AbdellahMohamed AbdellahMohamed Abdellah, Kaibo Zheng, and Tõnu Pullerits
“Electron Relaxation in the CdElectron Relaxation in the CdElectron Relaxation in the CdElectron Relaxation in the CdSe Quantum DotsSe Quantum DotsSe Quantum DotsSe Quantum Dots----ZnO Composite: ZnO Composite: ZnO Composite: ZnO Composite: Prospects for Photovoltaic ApplicationsProspects for Photovoltaic ApplicationsProspects for Photovoltaic ApplicationsProspects for Photovoltaic Applications”
Scientific Reports, 4, (2014201420142014), DOI: 10.1038/srep07244.
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
xi
Abbreviations and symbols
PVsPVsPVsPVs Photovoltaics 1111ststststG PVsG PVsG PVsG PVs First generation photovoltaics 2222ndndndndG PVsG PVsG PVsG PVs Second generation photovoltaics 3333ededededGPVsGPVsGPVsGPVs Third generation photovoltaics DSSCsDSSCsDSSCsDSSCs Dye-sensitized solar cells BHJBHJBHJBHJ Bulk heterojunction QDSCsQDSCsQDSCsQDSCs Quantum dots solar cells QDSSCsQDSSCsQDSSCsQDSSCs Quantum dots-sensitized solar cells OSCsOSCsOSCsOSCs Organic solar cells NCsNCsNCsNCs Nanocrystals QDsQDsQDsQDs Quantum dots VBVBVBVB Valence band VBMVBMVBMVBM Valence band maximum CBCBCBCB Conduction band CBMCBMCBMCBM Conduction band minimum UVUVUVUV Ultra violet VisVisVisVis Visible PLPLPLPL Photoluminescence FWHMFWHMFWHMFWHM Full width at half maximum QYQYQYQY Quantum yield EBEEBEEBEEBE Exciton binding energy MEGMEGMEGMEG Multiple exciton generation SCsSCsSCsSCs Solar cells MOMOMOMO Metal oxide CSQDsCSQDsCSQDsCSQDs Core–shell quantum dots CSSCSSCSSCSS Core–shell–shell TOPOTOPOTOPOTOPO Tri-n-octylphosphine oxide OAOAOAOA Oleic acid LEDLEDLEDLED Light-emitting-diodes TVsTVsTVsTVs televisions NWsNWsNWsNWs Nanowires NPsNPsNPsNPs Nanoparticles TRTRTRTR Time-resolved TATATATA Transient absorption PDPDPDPD Photo diode EDXEDXEDXEDX Energy-dispersive X-ray spectroscopy
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
xii
⟨�⟩ mean number of excited electron-hole pairs per QD XRDXRDXRDXRD X-ray diffraction TOPTOPTOPTOP Tri-n-octylphosphine MPAMPAMPAMPA Mercaptopropionic acid TMAOHTMAOHTMAOHTMAOH Tetramethylammonium hydroxide ODEODEODEODE 1-octadecane HMTAHMTAHMTAHMTA Hexamethylenetetramine SEMSEMSEMSEM Scanning electron microscopy HRHRHRHR----TEMTEMTEMTEM High resolution transmission electron microscopy AFMAFMAFMAFM Atomic force microscopy FTOFTOFTOFTO Fluorine-doped SnO2 TCSPCTCSPCTCSPCTCSPC Time-correlated single photon counting nsnsnsns Nanosecond pspspsps Picosecond fsfsfsfs Femtosecond nmnmnmnm Nanometer eVeVeVeV Electron volt AugRAugRAugRAugR Auger recombination rrrr Particle radius EEEEg,eff.g,eff.g,eff.g,eff. Effective band gap EEEEgggg((((∞)))) Bulk band gap mmmmeeee Electron effective mass mmmmhhhh Hole effective mass ε Relative permittivity DOSDOSDOSDOS Density of states αBBBB Bohr exciton radius ε0000 Free vacuum permittivity μ Reduced mass KEKEKEKE Kinetic energy τRRRR Radiative lifetimes τnonRnonRnonRnonR Nonradiative lifetimes τObObObOb Observed lifetime THzTHzTHzTHz Terahertz spectroscopy KKKK injinjinjinj Electron injection rate ΔGGGG Free energy change ΔEEEEelelelel Electron energy difference ΔEEEEhhhh Hole energy difference ΔEEEECCCC Coulombic energy change CTSCTSCTSCTS Charge transfer state PLEPLEPLEPLE Photoluminescence excitation
Ultrafast Photoinduced Processes in Core and Core–Shell Quantum Dots for Solar cell Applications
xiii
PEEPEEPEEPEE Photoinduced emission enhancement λ Reorganizational energy IAIAIAIA----QDsQDsQDsQDs Indirect attached QDs to MO RRRR The fraction of IA-QDs DADADADA----QDsQDsQDsQDs Direct attached QDs to MO FRETFRETFRETFRET Fӧrster resonance energy transfer IPCEIPCEIPCEIPCE Incident photon-to-electron conversion efficiency kkkkETETETET Energy transfer rate RRRRDADADADA Donor–acceptor distance 1/1/1/1/RRRR6666 Distance term LLLLDDDD Diffusion length BBBB Dispersion factor β Distance exponential dependence factor ηinjinjinjinj Electron injection efficiency ηEC Electron collection efficiency ηhhhh Hole collection efficiency
Introduction
1
Chapter 1: Chapter 1: Chapter 1: Chapter 1: IntroductionIntroductionIntroductionIntroduction
1.1 Sustainable energy source1.1 Sustainable energy source1.1 Sustainable energy source1.1 Sustainable energy sourcessss::::
In the modern society, energy is the engine of economic development. More than 85%
of the global energy consumption comes from the fossil fuels such as oil, natural gas,
and coal. During 2013, the world consumed about 4200 million tons of oil, 3100
million tons of oil equivalent of natural gas, and 3900 million tons of oil equivalent of
coal according to BP statistical review report.1 Burning these fossil fuels as an energy
source has a huge deteriorating impact on the environment.2 Due to the shortage and
pollution from the fossil energy sources, governments and scientists in many countries
have been making effort to find an alternative energy sources “sustainable energy
sources”. There are several types of sustainable energy sources such as nuclear,
hydroelectric, wind, geothermal, and solar (photovoltaics).3
Harvesting the energy from Sun has many advantages. Compared to nuclear power
plants, solar sources (see figure 1.1A) are technically facile and safe. Moreover, they are
free of gas pollution and territory limitation, as long as solar radiation is sufficient in
that area. It is reported that 1% of the solar power is more than enough for the total
global energy consumption if it could be converted into electricity or fuel.4 Over the
past years, conversion of light into the electrical energy has been explored using
different materials. The first generation of photovoltaics (1stG) includes semiconductor
solar cells mainly based on Si material with high efficiency. The second generation
(2ndG) of solar cells was aimed to reduce the high costs of the first generation solar cells
through the utilization of thin film technology with the challenge of increasing the thin
film absorption to compensate for the reduced thickness in the photoactive layers. The
2ndG PVs are considered as low cost/low efficiency devices compared to 1stG
counterparts. The third generation (3edG) of PVs should combine the cheap material
processing typical for the 2ndG with the high conversion efficiency of the first
generation. The 3rdG is based mainly on nanostructured materials with three major
types that have dominated research in recent years (see figure 1.1B): (a) dye-sensitized
solar cells (DSSCs), (b) bulk heterojunction (BHJ) PV cells or organic PV cells, and (c)
quantum dot solar cells (QDSCs). The later considered as “The Next Big Thing” in
photovoltaics.5
Introduction
2
Figure 1.1: A) Solar radiation spectrum outside of the atmosphere (yellow area)
compared to the sea-level radiation (red area)6, and B) reported efficiency of
quantum dot solar cells (QDSCs, black) compared to dye sensitized solar cells
(DSSCs, red) and various types of organic solar cells (OSCs, blue)7.
1.2 Quantum Dot (QD): 1.2 Quantum Dot (QD): 1.2 Quantum Dot (QD): 1.2 Quantum Dot (QD):
Quantum dot (QD) is a semiconductor nanocrystal (NC) with a size of 2-10 nm. In
the bulk semiconductor the charge carriers can be considered as being free particles
with a modified mass (the so-called effective mass). When the size of material
approaches the exciton Bohr radius (typically several nanometers), the picture changes
into the “particle-in-box” problem. The term “dot” in quantum dot refers to
confinement of electrons and holes in all three dimensions. This is an extension of
quantum “wires” and quantum “wells” that confine excitons in one and two
dimensions, respectively (see figure 1.2A).
In semiconductors, exciton (electron-hole pair) is created after the absorption of a
photon with energy above the semiconductor band gap energy. Band gap is the
minimum energy difference between the highest occupied state in the valence band
(VBM) and the lowest occupied state in the conduction band (CBM). Depending on
the electron momentum at the CBM and VBM, the band gap can be either direct or
indirect. Most of the semiconductors have direct band gap where the CBM and VBM
occur at the same value of electron momentum (CdSe, CdTe, and many others). On
the other hand some semiconductors, such as Si, have the indirect band gap where the
CBM and VBM occur at different values of electron/hole momenta.
Introduction
3
Figure 1.2: A) Quantum well (2D), quantum wire (1D) and quantum dot (0D)8,
and B) quantum dot size related to the conduction band and valence band.
Even though the initial theory behind the exciton has existed since the 1930’s9-11 it
was not until the 1980’s that researchers began to focus on the effect of quantum
confinement on excitons in semiconductor materials.12 In the 1970’s, advances in
microfabrication led to quantum confinement in two-dimensional wells13, eight years
later was reported the first demonstration of one-dimensional wires.14 Finally, about 30
years ago in the former Soviet Union, Aleksey Ekimov12 and Alexander Efros15 explained
the spectral differences of what appeared to be tiny particles of variable sizes. One to
two years later, Louis Brus16 in the United States and Arnim Henglein17 in Germany
discovered striking color change of II-VI semiconductor nanoparticles grown as
aqueous colloidal suspensions.
Introduction
4
1.3 Quantum Dot (QD) properties:1.3 Quantum Dot (QD) properties:1.3 Quantum Dot (QD) properties:1.3 Quantum Dot (QD) properties:
Due to the quantum confinement effect, the energy levels are quantized depending on
the QD’s size.18 As the NC’s size decrease (smaller than exciton radius), the quantum
confinement becomes more dominant, and consequently the QD properties will
change. As a result of the quantum confinement effect, the band gap becomes wider
(see figure 1.2 B) and QDs therefore absorb at higher energies. Also the oscillator
strength is concentrated into a few transitions as a result of changes in the density of
electronic states from the bulk size to the QD size. The QDs’ photoluminescence (PL)
depends on the QD’s size as well, following the band gap changes19 (see figure 1.3A).
An interesting feature of semiconductor QDs is the symmetric and relatively narrow
emission peak redshifted with respect to the corresponding absorption peak. The red
shift of the emission is known as Stokes shift. Stokes shift is the difference between
positions of the band maxima of the absorption and emission spectra in wavelength or
frequency unit. This difference comes from the fact that, after the excitation, the QDs
tend to relax by emitting photons with some energy losing as dissipation of thermal
phonons in a crystal lattice. PL wavelength depends on the QD material and size, as
stated before (see figure 1.2 B). The PL from QDs usually feature a high quantum yield
(QY ≈ 0.2–0.9).20 Moreover, QDs excel in high molar extinction coefficients, better
photostability compared with common standard fluorophores, as well as the high
resistance to photo- and chemical degradation.21-23
In QDs, the excitons (electron-hole pairs) occupy discrete energy states similar to
electrons of a single atom and that is why the QDs are sometimes referred to as the
“artificial atoms”18 (see figure 1.3 A). After excitation with sufficient energy photon, the
QDs’ electrons will be excited from the valence band (VB) to the conduction band
(CB) leaving the positive quasi-particles holes in the VB. Holes can be considered as a
mobile positive charge in the VB. Then both the electrons and holes rapidly lose their
energy and jump to levels near the bottom of their conduction band (CBM) and the
top of their valence band (VBM), respectively (see figure 1.3 A). As the electrons relax
across the band gap to recombine with the holes, the energy released by recombination
from the excited state to the ground state can be calculated as the sum of the electron
and hole confinement energy, the exciton binding energy (EBE), and the band gap
energy.24 In QDs, a photon with energy twice higher than the band gap can create
multiple excitons, this phenomenon is called “multiple exciton generation” (MEG) (see
Introduction
5
figure 1.3 B).25-26 The same phenomenon exists also in bulk semiconductors. Efficient
formation of more than one electron-hole pair out of one incident high energy photon
is potentially very important from solar cell application point of view. Recently, several
studies have proven the successful utilization of MEG to enhance the quantum
efficiency of QD-sensitized solar cells (SCs) based on QD-metal oxide (MO) system.27-
28
Figure 1.3: A) Excitation, relaxation (cooling) and electron-hole recombination in
QD, and B) multiple exciton generation in QD 1) excitation with high energy
photon, 2) the electron relax to the CBM releasing its energy to process 3, and 3)
creating another exciton by using the energy of process 2).
1.4 Core1.4 Core1.4 Core1.4 Core––––shell quantum dots (CSQDs): shell quantum dots (CSQDs): shell quantum dots (CSQDs): shell quantum dots (CSQDs):
As the crystal becomes smaller, the proportion of the atoms on the surface increases,
which has an impact on the nanoparticle properties. In general, during the synthesis of
QDs, some atoms on the crystal facet are incompletely bonded within the crystal lattice
which leads to one or more of “dangling bonds”.29 Most nanocrystals are highly faceted,
what leads to an array of dangling bonds with a band energy level similar to the crystal
itself.30-31 These states could work as a trap states if their energy is located within the
QD band gap resulting in: i) reducing the overlap between the electron and hole, and
ii) increasing the nonradiative depopulation pathways of the excited states. One way
that minimize the surface states, is by passivating the nanocrystals surface using organic
ligands (capping agents) like tri-n-octylphosphine oxide (TOPO) or oleic acid (OA).
Capping agents adsorb to the nanocrystal surface through dative ligand–metal bonds
between the ligand active group and the metal atoms on the nanocrystal surface.
{
CBM
VBM
{CB
VB
QDQDQDQD
hν Electron-hole recombination
AAAA
hν>2Eg
1
2
Eg3
BBBB
MEG in QDMEG in QDMEG in QDMEG in QD
Introduction
6
Nonpolar end group ligands solubilize the nanocrystals in nonpolar solvents and the
same holds for polar end group ligands in case of polar solvent.29
Another more effective way to passivate the surface defect states is to coat the
semiconductor nanocrystal with an inorganic shell with higher band gap thereby
insulating the excitons in the core from the surface states. In other words, core–shell
quantum dots (CSQDs) can be broadly defined as comprising core (inner
semiconductor) and a shell (outer semiconductor). In solid state devices, this process is
quite simple, as overgrowth of an inorganic layer with a wider band gap can be readily
achieved with complete surface passivation. However, the task is more challenging in
preparing colloidal CSQDs such as CdSe–ZnS and CdSe–CdS CSQDs with sufficient
and stable PL. CSQDs can be categorized based on the band gaps of both the core and
the shell materials into many types, each useful for different applications (see chapter 4
for more details).32
1.5 Quantum dots applications: 1.5 Quantum dots applications: 1.5 Quantum dots applications: 1.5 Quantum dots applications:
Both neat core and CSQDs are gradually attracting more and more attention, since
these nanocrystals have emerged at the frontier of material science and many other
fields, such as biomedicals, pharmaceuticals, optics, and catalysis. In the next
subsections, some of the QDs important applications will be listed.
1.5.11.5.11.5.11.5.1 QDs for biomedical applications:QDs for biomedical applications:QDs for biomedical applications:QDs for biomedical applications: QDs are mainly used for controlled drug
delivery33, for bioimaging34, cell labeling35, as biosensors35, and in tissue
engineering applications.36
1.5.21.5.21.5.21.5.2 QDs for light emitting diodes (LED), electricity inQDs for light emitting diodes (LED), electricity inQDs for light emitting diodes (LED), electricity inQDs for light emitting diodes (LED), electricity in––––light out: light out: light out: light out: one
strikingly beautiful aspect of colloidal QDs is the way their emission colors
change with their size (band gap). This allows QDs to be used as ultra-efficient
light-emitting-diodes. Recently, Sony Corporation of Tokyo announced that
using QDs for flat-screen televisions (TVs) will transmit more richly colored
images than other TVs on the market.37
1.5.31.5.31.5.31.5.3 QDs for solar cells (SQDs for solar cells (SQDs for solar cells (SQDs for solar cells (SCs), light inCs), light inCs), light inCs), light in––––electricity out:electricity out:electricity out:electricity out: “No signs of abating”.38
Colloidal QDs films form the core of solar cells devices. Figure 1.5 shows the
principle of operation of three types of solar cells that employ semiconductor
QDs as light harvesters.39 In these types, the QDs film absorb the light to
produce electron-hole pair, which must then be separated and extracted at the
opposite electrodes.38 Since, the first report on infrared colloidal QD solar cells
Introduction
7
on 200540 much progress has been made towards technologically relevant
efficiencies. Efforts have been made to improve the efficiency of QD based
solar cells leading to enhance the efficiency from 2% in 200841 to around 3%
in 2009-201042-43, 4.6% in 2011 for metal/QDs device44, and 6% in 2011 as
well by optimizing the device architecture and its constituent materials.45
Recently, by engineering the QDs band alignment both the performance and
the stability of the QD (semiconductor bulk heterojunction) solar cells were
improved (certified efficiency ~ 8.6%).46
Figure 1.5: Schematic diagram of QDs based solar cells5 i) semiconductor
heterojunction SCs, ii) polymer/QDs hybrid SCs, and iii) QDs-sensitized SCs.
1.6 Quantum dots toxicity: 1.6 Quantum dots toxicity: 1.6 Quantum dots toxicity: 1.6 Quantum dots toxicity:
QD toxicity has been the major roadblock for using these materials in clinical research
and applications. Along with composition, the physical and surface characteristics (size,
shape, surface charge, and capping agent) of the QDs play the major role in the toxicity.
In 2006, Nawrot et al. have reviewed current understanding of the impact of cadmium
(Cd) on human health.47 Current understanding states that environmental exposure to
Cd increases total mortality in a continuous fashion, without any evidence of critical
dosage. They have noted that tubular kidney starts at urinary Cd concentrations
between 0.5 and 2 μg urinary Cd per g creatinine. In addition, recent investigation
focusing on bone effects showed increased risk of osteoporosis even at urinary Cd as
low as 1 μg Cd per g creatinine.48 For the pulmonary toxicity, which refers to the side
effect on the lungs developed by interaction with nanoparticles. This is important for
work place exposures resulting from preparation of large quantities of nanomaterials as
powders that can be dispersed to the air. Fortunately, most colloidal QDs like those
used in this thesis do not form dry powders. Even upon solvent evaporation they
typically remain waxy due to the large amount of organic molecules encapsulating them
Introduction
8
(capping agent). In general working with QDs is safe provided that one shows care and
respect starting from the synthesis until using them for different application and final
disposal.
Experimental methods
9
Chapter 2: Chapter 2: Chapter 2: Chapter 2: Experimental methodsExperimental methodsExperimental methodsExperimental methods
In this chapter, the preparation of different samples and the experimental methods used
in this thesis are presented.
2.1 Materials:2.1 Materials:2.1 Materials:2.1 Materials:
All chemicals used in the synthesis were purchased from Sigma–Aldrich without further
purification. Cadmium oxide (99.5%), selenium (>99.5%), oleic acid (OA, >99%),
and trioctylphospine (TOP, >90%) were used to prepare neat CdSe quantum dots
(QDs). In addition, zinc acetate (99%) and sulfur (99%) for gradient Cd1-xZnxSe1-ySy
core–shell QDs. Mercaptopropionic acid (MPA, >95%) and tetramethylammonium
hydroxide (TMAOH, 25% wt. in methanol) were used to exchange the ligand of QDs
for sensitization on metal oxide (MO). Solvents used in the QD synthesis and ligand
exchange included 1-octadecane (ODE, 90%), toluene (anhydrous, 99.8%), methanol
(anhydrous, 99.8%), acetone (HPLC, >99.8%), ethanol (99.7%). Zinc acetate
(>99%), ethylamine (>99.5%) and 2-methoxyethanol (anhydrous, 99.8%) were used
to prepare ZnO seed layer for nanowires synthesis, and the precursors for ZnO NWs
growth included zinc nitrate hexahydrate (>99%) and hexamethylenetetramine
(HMTA, >99%). ZnO and TiO2 nanoparticles (NPs) were purchased from Sigma–
Aldrich with average particle size (<35 nm and 15-20 nm, respectively). For p-type
NiO mesoporous films, anhydrous NiCl2 and polyethyleneoxide–polypropyleneoxide–
polyethyleneoxide triblock co-polymers (F108) were purchased from Sigma–Aldrich
without further purification as well.
2.22.22.22.2 Synthesis of Synthesis of Synthesis of Synthesis of neat neat neat neat CdSe QDsCdSe QDsCdSe QDsCdSe QDs::::
In a three-neck flask, a 70 ml octadecene ODE solution containing 5.54 g OA and
0.51 g CdO was first heated to 180 °C to form a clear solution under N2 atmosphere.
1.3 mmol Se powder and 0.5 g trioctylphosphine (TOP) were dissolved in 10 ml ODE
by stirring for 1 hour under N2 atmosphere as well. The obtained TOP-Se solution was
quickly injected in the three-neck flask.49 During the injection of TOP-Se solution, the
Cd2+ precursor solution was heated up to 180, 200, 220, 240, 280 and 320 °C to obtain
different sizes of QDs. After 2 minutes reaction, the flask was removed from the heater
and cooled down to room temperature. Finally, methanol and acetone were added to
Experimental methods
10
precipitate the QDs, which were consequently redissolved in toluene. The purification
procedures were repeated twice in order to remove unreacted materials before using the
QDs for any measurements.
2.32.32.32.3 Synthesis ofSynthesis ofSynthesis ofSynthesis of gradient gradient gradient gradient CdCdCdCd1111----xxxxZnZnZnZnxxxxSeSeSeSe1111----yyyySSSSyyyy CSCSCSCSQDs:QDs:QDs:QDs:
Cd1-xZnxSe1-ySy gradient CSQDs were prepared via single-step hot injection method.
Typically, 0.4 mmol (0.05 g) of CdO, 4.0 mmol (0.88 g) of zinc acetate, 17.6 mmol
of oleic acid and 20 ml of 1-octadecene (ODE) were placed in a round flask. The
mixture then heated to 150 °C, degased for 20 min, filled with N2 gas, and further
heated to 310 °C to obtain a clear solution of Cd- and Zn-oleate. At this temperature
(injection temperature), 0.4 mmol (0.03 g) of Se powder, and 4.0 mmol (0.13 g) of
sulfur powder both dissolved in 3.0 ml TOP under N2 gas were quickly injected into
the cationic oleate reaction flask. After the injection the growth temperature was
adjusted to 300 °C for different shell growth time 5sec, 1, 3, 5, 10, and 15 min where
part of the reaction mixture was cooled down using ice bath to eliminate the QD’s
growth. As prepared QDs were purified using 1:3 chloroform-acetone mixture twice
and finally the purified QDs were redispersed in hexane.20
2.42.42.42.4 QDs surface QDs surface QDs surface QDs surface ligand ligand ligand ligand exchangeexchangeexchangeexchange::::
Attachment of the QDs to the MO was carried out by exchanging the capping agent
of as-obtained oleic acid-capped QDs with MPA linker. MPA is a bifunctional
molecule to link the QD to the MO via its two terminals (-SH and –COOH).
Therefore, 1.0 ml oleic acid-capped QDs with the concentration of 0.4 mM was mixed
with 0.1 ml MPA and 1.0 ml acetone. The mixture was stirred for 30 min. Afterwards
0.5 ml of ethanol was added to the mixture, which was then stirred another 15 min.
The resulting reactants were centrifuged at 3500 rpm for 5 min and the supernatant
was discarded. The resulting precipitates were redissolved in ethanol. Finally, TMAOH
was added drop wisely, so that a totally clear solution containing MPA-capped QDs
was formed. In order to prepare MO NPs film, purchased ZnO NPs, and TiO2 NPs
suspension was doctor-bladed on a glass substrate then annealed at 450 °C for 30 min
and then dried at room temperature. Then the MO films were immersed into MPA-
capped QDs ethanol solution in the dark. Afterwards, the films were washed
thoroughly with ethanol and dried using N2 gas. In paper VI, the linker exchange was
carried out on the substrate directly. Where, two sizes of QDs were mixed with 1:1
Experimental methods
11
volume ratio, and then spin-coated onto a glass substrate at a spinning rate of 1000
rpm for 30 s. Afterwards 10% mercaptopropionic acid (MPA) in methanol was spin-
coated with the same condition to exchange the oleic acid capping agent of the as-
obtained QDs. Then the film was rinsed using methanol and toluene to remove
excessive QDs and MPA. This deposition process is repeated for several times to form
a thick layer of QDs.
2.52.52.52.5 ZnO NWs and NiO mZnO NWs and NiO mZnO NWs and NiO mZnO NWs and NiO mesoporous filmesoporous filmesoporous filmesoporous filmssss preparationpreparationpreparationpreparation::::
The synthesis of n-type ZnO NWs followed the widely known hydrothermal method.50
Briefly, 50 mM solution of zinc acetate dihydrate (Zn(CH3COO)2∙2H2O) and
ethanolamine in 2-methoxyethanol was spin-coated onto a fused silica substrate for 3
times and then sintered at 450 °C for 30 min in ambient to form a thin seed layer. The
hydrothermal growth of highly oriented ZnO NWs on the seeded substrate was carried
out at 92.5 °C in aqueous solution containing 20 mM HMTA and zinc nitrate. After
the growth, the sample was carefully rinsed in deionized water and dried at 100 °C. For
p-type NiO MO, by dissolving anhydrous NiCl2 (1.0 g) and polyethyleneoxide–
polypropyleneoxide–polyethyleneoxide triblock co-polymers F108 (1.0 g) into a
mixture of Milli-Q water (12.0 g) and ethanol (24.0 g). The solution was kept in room
temperature for 1 day for stabilization, and then centrifuged. The obtained supernatant
solution was doctor-bladed on a glass substrate and dried at room temperature. The
dried film was then calcined in air at 400 °C for 0.5 h.
2.62.62.62.6 QDs QDs QDs QDs characterizationcharacterizationcharacterizationcharacterization::::
Steady-state absorption and emission spectra were measured using an Agilent 845x
spectrophotometer and Spex 1681 spectrometer, respectively. The photoluminescence
quantum yield (PL QY) of the QDs was measured and estimated by comparing the
QDs’ PL intensities with that of standard rhodamine 6G dye at the same optical density
(0.07).51 The morphologies of QDs studied in this thesis were characterized via high
resolution analytical transmission electron microscopy (HR-TEM, JEOL 3000F
microscope equipped with an Oxford SDD x-ray analyzer) in order to obtain the
average size of the QDs. Chemical composition of CSQDs was estimated from the
energy-dispersive X-ray spectroscopy (EDX) spectra corresponding to the HR-TEM
images. Here TEM is operated in scanning transmission electron microscopy (STEM)
mode probing the information of the local chemical composition of the sample. The
Experimental methods
12
morphology of multi-sized QD (paper VI) assemblies was imaged in the tapping mode
by an atomic force microscopy (AFM) (AFM 5500 System, Agilent Technologies).
2.72.72.72.7 Solar cell device fabrication:Solar cell device fabrication:Solar cell device fabrication:Solar cell device fabrication:
In paper VIII to fabricate the photoanode for solar cells, TiO2 paste (Ti-Nanoxide HT)
was coated on the surface of fluorine-doped SnO2 (FTO) by doctor-blading technique.
After annealing at 450 °C for one hour, the obtained TiO2 mesoporous film is suitable
for QD sensitization. The sensitization time was varied for different QDs to keep the
same optical density. Finally, freshly prepared photoanode was scratched to area ~ 0.25
cm2. In order to complete the solar cell, 1.0 M Na2S/1.0 M S solution used as an
electrolyte and FTO glass coated with 200 Å Platinum was used as a cathode.52
2.2.2.2.8888 Transient absorption spectroscopy (TA):Transient absorption spectroscopy (TA):Transient absorption spectroscopy (TA):Transient absorption spectroscopy (TA):
Transient absorption measurements were carried out on a femtosecond laser setup
based on the MaiTai-pumped Spitfire Pro XP (Spectra Physics) with the central output
wavelength of 800 nm and 1 kHz repetition rate delivering ~80 fs pulses. The beam
was split into two parts: one for pumping a collinear optical parametric amplifier
(TOPAS-C, Light Conversion) to generate the pump beam (470 nm), and the second
one was either focused onto a CaF2 crystal or a thin sapphire plate to generate a white
light continuum (for transient spectra measurements), or was used for pumping a
second TOPAS-C to generate narrow-band probe pulses at certain wavelength
depending on the purpose of the measurement (for kinetics measurements). The delay
between the pump and probe pulses was introduced by a delay line. The mutual
polarization between pump and probe beams was set to the magic angle (54.7°) by
placing a Berek compensator in the pump beam. Generally, we used thin-film samples
of QDs on MO (OD ~ 0.05) and colloidal samples in the 1-mm quartz cell (OD
between 0.2 ~0.4). During measurements the film samples were kept in N2 atmosphere
to avoid possible photodegradation (see figure 2.1).
Experimental methods
13
Figure 2.1 Schematic picture of the fs TA setup with single wavelength probe and/or
white light (visible) probe. In this setup laser light (800 nm) is emitted and split into
two parts; one for pump (green line through Topas 2) and the other for probe (red
line for white light or blue line through Topas 1). Every second pulse of the pump
light is blocked by the chopper (the pump intensity was controlled by using PD1).
The pump extra path can be used to increase the traveled distance of the pump (used
for single wavelength kinetics experiments). For white light probe (TA spectra), the
beam is first directed on the delay-stage to increase the distance that the probe light
travels compared to the pump beam. Secondly, the white light is generated using a
CaF2 crystal or a thin sapphire plate. For single wavelength kinetics, the probe light
is converted in Topas 1 then directed on the delay stage. For both cases (white light
probe or single wavelength probe), the probe light is then split into a probe and
reference. The probe is overlapped with the pump on the sample and then directed
to the detector (monochromator for white light or PD2 for single wavelength). The
reference bypasses the sample and is directed to the PD3. The difference spectrum
can be created by collecting alternating spectra with pump on and pump off.
2.2.2.2.9999 TimeTimeTimeTime----resolved PL spectroscopy (TRPL):resolved PL spectroscopy (TRPL):resolved PL spectroscopy (TRPL):resolved PL spectroscopy (TRPL):
2.9.1 TimeTimeTimeTime----correlated single photon countingcorrelated single photon countingcorrelated single photon countingcorrelated single photon counting (TCSPC)(TCSPC)(TCSPC)(TCSPC): Time-resolved PL
measurements were performed using a time-correlated single-photon counting device
(PicoQuant). A pulsed diode laser at different repetition rates was used to excite the
Experimental methods
14
sample at 438 nm. The pulse duration of the laser was about 200 ps. The PL from the
sample was filtered using long-pass filters from 520 nm to pick up only band edge
emission. The emitted photons were focused onto a fast avalanche photodiode (SPAD,
Micro Photon Device). The response time of the photodiode was <50 ps. The
excitation photon flux was controlled using neutral filters with different optical density.
2.9.2 StStStStrrrreak cameraeak cameraeak cameraeak camera: here the laser source for the time-resolved photoluminescence
setup is a titanium:sapphire passively mode-locked femtosecond laser (Spectra-Physics,
Tsunami), emitting at 820 nm with 80 MHz repetition rate and 150 fs pulse length.
In order to exclude the possible photocharging process in QDs, we also measured decay
kinetics of QDs with different pump repetition rates (80 MHz to 1.6 MHz) tuned by
a pulse picker keeping the pulse energy unchanged. The laser pulses were frequency-
doubled to 410 nm by a second-harmonic generator (Photop technologies, Tripler TP-
2000B). Time-resolved photoluminescence spectra were detected in a picosecond
streak camera (C6860, Hamamatsu, time resolution < 1 ps) coupled to a Chromex
spectrograph, triggered by the Ti:sapphire laser. A long-pass filter from 490 nm was
used in front of the spectrograph to cut off the scattering from the excitation pulses.
2.2.2.2.10101010 TimeTimeTimeTime----resolved terahertz spectroscopy (THz):resolved terahertz spectroscopy (THz):resolved terahertz spectroscopy (THz):resolved terahertz spectroscopy (THz):
The same laser system used in TA measurements was utilized for THz spectroscopy.
The laser beam was split into three. The first beam generates THz radiation by optical
rectification in a 1 mm thick (110) ZnTe crystal. The second beam was used in another
(110) ZnTe crystal for detection of THz pulses via electro-optical sampling. The third
beam seeds an OPA (Topas) generating 529 nm pulses used for sample photoexcitation
with a fluence of 6.3×1014 photons/cm2/pulse (mean number of excited electron-hole
pairs per QD, ⟨�⟩ = 1.2). To avoid absorption of THz radiation due to water vapor
and possible photodegradation of the sample, the THz apparatus was placed in a pure
nitrogen atmosphere.
2.2.2.2.11111111 XXXX----ray ray ray ray diffractiondiffractiondiffractiondiffraction (XRD)(XRD)(XRD)(XRD)::::
XRD experiments were carried out at the Beamline I711, in MAX IV Laboratory. The
energy of the incident X-ray is 12.5 keV (wavelength 0.99 Å). For the sample
preparation, 0.5 mm glass capillaries with the colloidal CSQDs solutions were gently
heated to fully evaporate the solvent. The XRD patterns were measured at room
temperature, in the atmosphere.
Exciton dynamics in QDs
15
Chapter 3: Chapter 3: Chapter 3: Chapter 3: Exciton dynamics in QDsExciton dynamics in QDsExciton dynamics in QDsExciton dynamics in QDs
3.1 Motivation3.1 Motivation3.1 Motivation3.1 Motivation::::
A better understanding of exciton dynamics in nanomaterials is thus important both
fundamentally and technologically53
In order to fully understand the dynamics of charge transfer from QD to metal oxide
(MO) in solar cell system, which is the main aim of the thesis, steady-state optical
properties of QD and the exciton dynamics within QD need to be discussed first. In
this chapter, we will start with the steady-state optical properties (absorption and
emission) of QDs. The ultrafast exciton dynamics within QD will be covered. We
continue with describing electron injection to metal oxide (MO)54, multiple electron
injection vs Auger recombination (AugR) to MO55, hole trapping56 by trap states and
hole injection57 to p-type MO. Finally energy transfer within CdSe QDs/MO system 58 and multi-sized CdSe QDs assembles 59 will be discussed.
3.2 3.2 3.2 3.2 SteadySteadySteadySteady----statestatestatestate absorption and emission: absorption and emission: absorption and emission: absorption and emission:
As we discussed in chapter 1, semiconductor optical properties are determined by the
electronic structure of the semiconductor. In QDs, the size (quantum confinement)
has a great effect on both optical absorption and photoluminescence (PL). As the size
of QDs decreases, blue shift in both optical absorption and PL occurs. This can be
accounted for using the particle-in-sphere model for a sphere with radius r:60
��,.� � = ���∞� + ����
��� � ���
+ ���
� − �.� �
�� , (1)
where, Eg(∞) is the bulk band gap, me and mh are the electron and hole effective masses
respectively, and ε is the relative permittivity of the semiconductor.
In eq. 1 the second term on the right hand side shows that the effective band gap is
inversely proportional to the square of the particle’s radius r and thus increases as the
size decreases, while the third term on the right hand side, due to electron-hole
Columbic attraction results in a decrease in the band gap with increasing particle radius.
However, for small particles (small r) the second term is dominating and thus the
effective band gap increases with decreasing r.53
Exciton dynamics in QDs
16
Quantum confinement becomes pronounced when the QD’s size is comparable or
smaller than the Bohr exciton radius (αB):
! = �"���
�#� , (2)
In eq. 2 ε and ε0 denote the relative permittivity of the semiconductor and the
permittivity of the vacuum, respectively, μ is the electron and hole reduced mass
$$� �$ + $��⁄ , and e is the electron charge. For example the Bohr radius of bulk
CdSe is ~ 5.6 nm.24 CdSe NCs with sizes comparable to this radius then exhibit a
noticeable blue-shifts in both absorption and PL spectra compared to the bulk spectra.24
Figure 3.1 A shows the absorption spectra of CdSe QDs with different sizes.56
The energy band of QDs would be split into discrete states due to the quantum
confinement both in CB and VB. In the absorption spectra, such discrete states would
induce pronounced exciton peaks. In particular, clear exciton peak would be observed
near the absorption band edge due to the electronic transition from the VBM to the
excitonic state that is located just below the CBM. The difference between the band gap
and the excitonic state energy emerges due to the electron-hole interaction and is
referred to as exciton-binding energy (EBE).24 The recorded EBE value of CdSe QDs,
for instance, is size dependent and can reach 1.0 eV for the 2.8 nm QDs size.24
Apart from absorption spectroscopy, we can also utilize photoluminescence (PL, see
Figure 3.1 B) to probe the excitonic states near the band edge or within the band gap
(i.e defect/trap states). For a typical NC, PL spectrum contain emission from both band
edge and trap states.56 The trap states which are located within the band gap form a
red-shifted PL band compared to the band edge emission (because of the reduced
transition energy between these states and the opposite band).61 The trap emission is
usually very broad because of various trap states with different properties exist. In
practice it is possible to passivate the surface trap states of QDs using organic capping
agent like oleic acid (OA),57 tri-n-octylphosphine oxide (TOPO),62 by surface
modification techniques63 or by growing a semiconductor shell around the core (core–
shell structure).64 This will result in enhanced band edge emission (discussed more in
chapter 4). Some other QDs were found to be weekly luminescent or even non-
luminescent at room temperature like PbI2 and CuS. This property is mainly due to
the indirect band gap65 character of these materials and the high density of internal
and/or trap states which act as PL quenchers.53
Exciton dynamics in QDs
17
Figure 3.1: A) Absorption spectra of CdSe QDs with different sizes in toluene56, B)
emission (PL) spectra from different sizes of CdSe QDs in toluene56, and C)
schematic illustrating the optical band edge absorption and the exciton binding
energy (EBE).
3.3: 3.3: 3.3: 3.3: Exciton dynamics:Exciton dynamics:Exciton dynamics:Exciton dynamics:
In QDs, absorption of a photon with energy larger than the QD band gap results in
excitation of an electron in the CB and a hole in the VB. The carriers are bound to
each other by Coulombic interaction and form an exciton due to large EBE. Initially,
within few tens of fs, an electronic dephasing takes place. Electronic dephasing is
considered as a dynamics process in which the energy is conserved while the phase
memory of the quantum state is lost. This process is considered as the fastest event that
excitons experience in semiconductors.66 For instance in CdSe QDs, the electronic
dephasing times at 15 K has been reported to be 85 fs based on three pulse photon
echo measurements.67 After the excitation with high energy photon, both electron and
hole have excessive kinetic energy (KE). Dissipation of this energy due to interaction
between electrons/holes and phonons on time scale of hundreds of fs is resulting in
AAAA BBBB
{ }VBVBVBVB
CBCBCBCB
{
Band gapOptical absorption
Exciton binding energy (EBE)
CCCC
400 450 500 550 600 650 700
0.2
0.4
0.6
0.8
1.0
1.2
1.4
No
rm.
Ab
s.
Wavelength (nm)
2.3 nm
2.6 nm
4.4 nm
7.0 nm
450 500 550 600 650 700 750 800 850
0.0
0.2
0.4
0.6
0.8
1.0
No
rm
. P
L
Wavelength (nm)
2.3 nm
2.6 nm
4.4 nm
7.0 nm
Exciton dynamics in QDs
18
intraband relaxation of the electron to the CBM and the hole to VBM. This intraband
relaxation is followed by radiative (emitting a photon)68 or nonradiative (producing
heat) recombination.69
Figure 3.2: Dynamic processes in QD: 1)
electron and/or hole relaxation through
electron-phonon coupling, 2) electron
trapping into trap states and the same may
occur for the hole (hole trap states), 3)
radiative and nonradiative band edge
electron-hole recombination, and 4) radiative
and nonradiative trapped electron-hole
recombination.
In semiconductor NCs, dynamic processes are generally more complicated compared
to the bulk semiconductor due to the presence of many band gap states. These states
are often referred to as surface states or trap states. Depending on the application of
interest for the semiconductor NCs, these surface states or trap states can be unwanted
or useful. For example, in the catalytic application, these states are useful70 where
electron or hole trapping will prevent the recombination and subsequent redox reaction
may occur using the trapped carriers. In contrast, for photovoltaics or luminescence
application these states are usually undesirable.71
In the QDs which are free from trap states, the electron and hole will primarily
recombine radiatively which leads to high PL quantum yield (PL QY), and exciton
lifetime on the order of a few to a few tens of ns (for direct band gap QD).54-55 On the
other hand, in the QDs with trap states, trapping process of electrons and/or holes by
these states becomes significant and occurs on time scale of a few ps to a few tens of ps
(see figure 3.2). As a consequence of high density of trap states, the band edge PL
intensity and the PL QY are very low.57 In QDs solar cells, especially QDs-sensitized
solar cells (QDSSCs), the trap states are usually induced by surface dangling bonds
which are always far from the interface to the acceptor and thus prevent the charge
transfer processes. Therefore, reduction of such trap states is very important for
photovoltaics application. Here, the charge separation plays a crucial role while the
trapping of the charge carriers is a strong competitive to the charge transfer to MO.
Exciton dynamics in QDs
19
More details about the charge (electron/hole) injection will be discussed in the
following sections.
In some cases, depending on the density and energy of the trap states, the trapped
carriers (electron and/or hole) can relax to deeper traps within the band gap. The
lifetime of the charge carrier in deep trap states can be as long as tens of ns72 to μs or
even longer.56 The experimentally observed lifetime of a given state τOb depends on
radiative and nonradiative lifetimes, τR and τnonR, respectively. For an ideal crystal where
the PL QY is high (~ 100%), τnonR is very long leading to τOb = τR. In reality, this is
seldom case where the observed lifetime has contributions from both radiative and
nonradiative lifetimes as follows:53
1 '()* = 1 '+* + 1 ',-,+* , (3)
./ 01 = '() '+* , (4)
In the rest of this chapter, the main objectives of papers I-IV will be presented in the
following order: Papers I and II contain work on the electron injection from CdSe QDs
to ZnO (MO).).).). Paper III analyses the hole trapping process and its long-lived
component, whereas the paper IV studies the hole injection from QDs to p-type MO.
In addition, exciton (electron-hole pair) transfer is presented in papers V and VI. As a
result of our work on neat CdSe QDs, a surface modification is necessary. Therefore,
chapter 4 mainly focus on Cd1-xZnxSe1-ySy gradient CSQDs and how controlling the
shell thickness improves the QD’s properties for solar cell applications.
Exciton dynamics in QDs
20
3333.4.4.4.4 Paper I “Electron injection from QDs to MO”Paper I “Electron injection from QDs to MO”Paper I “Electron injection from QDs to MO”Paper I “Electron injection from QDs to MO”: : : :
Studies of electron injection from QDs to MOs by using standard techniques (pump-
probe in the visible range, time-resolved PL) bring an ambiguity in interpretation. A
depopulation of QDs can be observed, however, without a possibility to distinguish
electron trapping from electron injection. Reported time scales of electron transfer
therefore varied from picoseconds up to nanoseconds, even for similar QD-MO
systems,54 and various interpretations of the observed kinetics can be found. In this
paper, ultrafast electron injection from CdSe QDs to ZnO NWs is observed to take
place on the picosecond time scale (3–12 ps) depending on the QD’s size by using
ultrafast time-resolved absorption technique (see figure 3.3 A). The electron injection
to the MO was further proved by terahertz (THz) spectroscopy technique where the
conductivity spectrum and rising signal confirms that the electrons arrive in the MO
in similar timescale as they leave the QDs (see figure 3.3 B).
Marcus theory of electron transfer: on 1992 Rudolph Marcus got the Nobel Prize in
chemistry for his theory of electron transfer.73 Tvrdy et al. used Marcus theory to
describe the electron injection rate from CdSe QDs to MOs as a function of the QD
sizes.74 In many-state Marcus model, where the electron is transferred from a discrete
molecule-like state in QD to a continuum of states in MO, the transfer rate can be
expressed as:
∫+∞
∞−
+∆+−= )
4
)(exp(
4
1)()(
2 22
kT
EG
kTEHEk
et λλ
πλρ
πh
, (5)
where, ρ(Ε) is the MO density of states (DOS), |34���|� is the electronic coupling
matrix element, 5 is the reorganizational energy, k is Boltzmann constant, T is the
temperature, and Δ7 is the free energy change. The free energy change ΔG can be
expressed as:
Δ7 = Δ�8 + Δ�9, (6)
where, ΔEel is the difference between the electron initial energy state (QD’s CB) and
the electron final state (MO’s CB) and the Coulombic term ΔEC arises from electron
and hole interaction. In other words, the electron energy difference acts as a driving
force for the electron transfer process where the Coulombic interaction energy acts
against the electron transfer process. Figure 3.3 C demonstrates that the electron
Exciton dynamics in QDs
21
injection rates with different driving forces induced by different QD sizes can be well
fitted by Marcus theory.
Figure 3.3: A) Normalized TA kinetics of neat QDs (dotted lines) and QDs-
sensitized ZnO NWs (solid lines) for different size of CdSe QDs, B) TA kinetics
compared to THz kinetics of (2.9 nm) QDs-ZnO NW, C) electron transfer rate (ket)
dependence on the free energy change (ΔG) described by Marcus theory, and D)
schematic illustrating the CTS model of the electron injection.
In addition to the fast injection (~ 6 ps) a slower kinetic component of about ~100
ps is clearly present in both TA and THz signal. This indicates the two-step electron
transfer via charge transfer state (CTS). Such model has been proposed previously in
dye-ZnO systems.75-76 In the CTS model, a fast electron injection is followed by a
slower process where the CTS dissociates and electrons are released to the NW bulk
(see figure 3.3 D). The ultrafast electron injection (~ ps) has important implications
for exploiting the multiple exciton generation (MEG) in QD-sensitized SCs. In this
context, the injection process has to compete with other fast loss channels, like Auger
recombination (AugR).
Exciton dynamics in QDs
22
3333....5555 Paper IPaper IPaper IPaper IIIII ““““Multiple exciMultiple exciMultiple exciMultiple exciton harvestington harvestington harvestington harvesting”: ”: ”: ”:
Performance–cost balancing is a crucial factor for solar cell expansion as a sustainable
source of energy. For example the single-junction SCs efficiency is restricted to be
below the Shockley–Queisser limit of about 32%.77 The Shockley–Queisser limit
originates from the fact that only photons with energy higher than or equal to the band
gap can be used to create excitons. Photons with energy less than the band gap will be
not absorbed and photons with energy higher than the band gap will create excitons
with excess energy which will be lossed as heat. QDs have a unique property which can
break the Shockley–Queisser limit via the so-called “multiple exciton generation”
(MEG). Instead of thermal relaxation, the excess energy can be used to excite one or
more electron-hole pairs. The harvesting of multiple electrons out of one excited QD
would increase the efficiency of SCs. Efficient MEGs in various materials of QDs and
QD–MO systems have been reported.27-28, 78-79 On the other hand, utilization of MEG
is limited by AugR where the recombination energy of one electron-hole pair is
transferred to electron or hole in the second electron-hole pair, which relaxes rapidly
via thermal relaxation.
In this paper, we study the electron injection under multiexciton conditions (high
excitation intensity). In paper I, we showed that the electron injection is very fast within
few to few tens of picoseconds for one electron-hole pair per QD (low excitation
intensity). Under multiexciton condition, a solid foundation for distinguishing the
competition between AugR and electron injection was revealed. Electron injection rates
from QDs to MOs strongly depend on the distance (shell thickness in this case)
between QDs and MOs. Three samples representing fast (sample F, no shell),
intermediate (sample I, thin shell), and slow (sample S, thick shell) electron injection
rate were chosen in this study (see figure 3.4 A).
A typical sign for multiple excitons in QDs is the rapid AugR55 leading to a kinetic
component which is significantly shorter than the single electron-hole pair
recombination on the nanosecond time scale.54 AugR contribution was determined
from the difference between TA decay kinetics under low and high excitation
conditions in the absence of the MO. Introducing the MO under the same excitation
conditions will affect the kinetics by the fast electron injection process. Thus for the
studied samples, AugR-electron injection lifetime ratio is 0.01, 1.2, and 4.5 for samples
F, I, and S, respectively.55
Exciton dynamics in QDs
23
Figure 3.4 B shows the effect of MO on the dynamics under high excitation intensity.
For sample S, AugR is more dominant where TA dynamics under different excitation
intensities are the same for attached and unattached QDs. Sample I presents a
combination of electron injection and AugR. At low excitation intensity, a fast TA
decay is due to electron injection. By increasing the intensity TA decay becomes faster
due to AugR. For instance, the mean lifetime changes from 60 ps at low excitation
(electron injection only, kinj) to 35 ps at high excitation (electron injection and AugR,
ktot) with AugR lifetime ~ 80 ps (the same in the absence of ZnO NWs ~ 73 ps).
Figure 3.4: A) Normalized TA kinetics of pure QDs (dotted lines) and sensitized
ZnO NWs (solid lines) for samples F, I, and S, B) normalized TA kinetics for
samples F, I, and S attached to ZnO NWs under different excitation intensity (all
excitation intensities are in μJ/cm2), C) schematic illustration of the 2nd electron
injection vs AugR, and D) electron injection rate dependence on QD size (orange
squares) fitted by Marcus theory (solid orange line) adopted from paper I; Auger
biexciton recombination rates (our results, dark cyan circles) and from ref 80 (dark
cyan triangles) fitted by D-p function (p = 4.9, dark cyan line).
Finally, the competition between electron injection and AugR is presented in sample
F. As the excitation intensity increases the TA decay becomes slower till excitation
intensity reaches ~ 700 μJ/cm2, then, TA signal decays faster. The slow decay (~ 50 ps)
can be understood as a competition between the second electron injection and trion
decay (positive trion is a QD contain two holes and one electron). Comparison of the
slow decay lifetime (~ 50 ps) and the reported trion lifetimes (~ 140 ps)81, indicates
Exciton dynamics in QDs
24
presence of an efficient injection of the second electron to MO. At higher intensity, the
TA dynamics becomes faster (see figure 3.4 B) due to AugR from more than doubly
excited QDs.
It is also essential to evaluate the size dependence of AugR rate. By the same methods,
AugR contribution can be extracted for different QD sizes. Like pervious results80, 82-83,
AugR lifetime becomes significantly shorter for smaller QDs. The obtained QD size
dependence of AugR rates can be well fitted by a D-p function (p = 4.9) which is in line
with previously reported dependences (see figure 3.4 D).84 We demonstrate that, the
multiple exciton harvesting efficiency changes significantly with QDs’ size. Already
within the narrow range of QD sizes (2–4 nm) the efficiency of the first exciton
harvesting can vary from 30% to 70% for this particular system (QD-linker-ZnO
NWs).
Exciton dynamics in QDs
25
3333....6666 Paper IPaper IPaper IPaper IIIIIIIII ““““UltraUltraUltraUltra----longlonglonglong----livedlivedlivedlived trapped holes in QDstrapped holes in QDstrapped holes in QDstrapped holes in QDs”:”:”:”:
After the formation of excitons, not all the carriers (electrons and holes) undergo a
prompt recombination. Some of them get trapped by defects and/or surface states. This
affects the dynamics of excitons85, reduces the PL yield86, and hinders the charge
transport.87 Recent studies have shown that the charge trapping is not always
detrimental to QDs application, and in some systems the trapped states can be used to
broaden the PL spectrum for potential application in white light-emitting-diodes.88-89
In this paper, we investigate the PL from the trapped states in oleic acid capped CdSe
QDs with various sizes (2.3-7.0 nm). The PL from the trapped states (due to localized
carriers) can be observed with red-shift to the PL from the band edge recombination
(due to delocalized carriers). In our investigation we found that the smaller the size, the
larger is the contribution of the red-shifted bands.90 We attribute this to the increase in
the surface-to-volume ratio with the decreasing size of the QDs, and therefore we
associate such red-shifted PL bands to surface trap states. We also found that this red-
shifted emission consists of at least two bands contributing to the surface states related
PL (see figure 3.6 A, PL1 and PL2), which indicates that more than one type of surface
states are radiative.
Furthermore, our photoluminescence excitation (PLE) measurements show that the
excitons above the band edge can get localized (trapped) at the surface and contribute
much more to the surface PL than the excitons excited at the band edge (see figure 3.6
B). This means that the trapping process is more efficient when the QDs are excited
above the band edge.91-92 Time-resolved PL (TRPL) helps us to understand the
dynamics of these trap states. Typically, localized carriers at shallow traps can delocalize
again at room temperature and contribute to the band edge PL, while the carriers at
deep traps are difficult to delocalize with lifetime longer than 2.5 μs (time window for
TRPL) in room temperature (see figure 3.6 C). Using ultrasensitive femtosecond
pump–nanosecond probe setup, a very long-lived component (> tens of μs) has been
observed. The photobleach signal suggests that the electrons remain delocalized and do
not recombine with the holes within few tens of ns (single exciton life time in CdSe
QDs), which means that the holes remain trapped on the microsecond time scale (see
figure 3.6 D). Our results add more evidence that the majority of the trapped carriers
in CdSe QDs are holes.
Exciton dynamics in QDs
26
Figure 3.6: A) Normalized PL from 2.3 nm CdSe QDs with red-shifted emission
from the trapped hole states (PL1 and PL2); inset: hole multi-trap states model, B)
PLE spectrum of 2.3 nm CdSe at different emission wavelengths, C) band edge (blue
line), trap-state emission (black line) decay obtained by using a sharp edge filter, and
the fit (red lines), and D) TA kinetics of CdSe QDs at different pump intensities;
inset: TA decay in early time scale (5-20 μs).
Exciton dynamics in QDs
27
3333....7777 Paper IPaper IPaper IPaper IVVVV ““““Hole injectionHole injectionHole injectionHole injection vsvsvsvs hole trappinghole trappinghole trappinghole trapping”:”:”:”:
The aim of this work is to evaluate the hole injection from QDs to p-type MO (namely,
NiO). Hole injection and hole trapping have similar spectroscopic signatures and it is
a challenge to separate them from each other. Furthermore the trapping process directly
interferes with injection hindering the efficient charge transfer.56 In addition, we
studied the dependence of hole injection on QD sizes and proved that the passivation
of hole traps by core–shell structure is beneficial for efficient hole injection.
In this work, we mainly used TRPL to analyze the hole dynamics in QDs because
other methods such as TA signals in visible spectral region is mainly sensitive to the
electrons in QDs’ CB. One difficulty to identify the hole injection process in QD-NiO
system is the competition from hole trapping induced by linker molecule exchange
from oleic acid (OA) to short chain thiol-based linker (e.g mercaptopropionic acid,
MPA).93 By comparing the TA and PL kinetics between OA-capped QDs and MPA-
capped QDs, we can prove the hole trapping process within 4 ps (see figure 3.7 A).94
However, the major fast hole trapping (~4 ps) induced by ligand dangling bond can be
significantly reduced by photoirradiation (known as photoinduced emission
enhancement “PEE”). This effect is commonly explained by surface passivation
induced by the chemical change of QD’s surface during the irradiation process.95
In this scenario, we can start to investigate the hole injection in QD-NiO system
after such “photoirradiation passivation” which would exclude the fast quenching
process by surface traps. The situation is different for QDs attached to NiO where we
used a global fitting of TA spectra in QD-NiO resulting in two components. The long-
lived component (~ 6 ns) can be assigned to exciton recombination whereas the fast
component (~ 200 ps) (see figure 3.7 B) can be explained by employing a charged-QD
model. Here, the hole injection from QD to MO will leave a charged-QD behind. If
negatively charged, the QD’s absorption edge will show a red shift on the scale of a few
meV.96 In our case, the difference between original and 10 meV shifted absorption
spectrum gives the TA fast component spectrum (see figure 3.7 B inset). This provides
an evidence for the charged QD model and at the same time directs towards the hole
injection to NiO, because the hole trapping itself does not lead to such behavior.
This fast component (~ 200 ps) is analogous to what we found in TRPL
measurements. The multi- exponential fitting of PL kinetics of QD-NiO exhibits an
additional fast decay component (~ 380 ps) compared to those of neat QDs samples.
Exciton dynamics in QDs
28
Therefore, it can be assigned to hole injection from QDs to NiO (see figure 3.7 C).
Similar to electron injection to ZnO NWs in paper I, we used Marcus theory (eq. 5)
to study the hole injection rates dependence on the QD’s size. We have modified the
free energy change term (ΔG) calculation (see eq. 7) to account for the hole properties:
∆7 = ∆�� + ∆�9, (7)
where ΔEh stands for the hole energy difference between the initial (QD’s VB) and the
final energy (MO’s VB) states. ΔEh has the same value since the VBM for CdSe is
independent of the QD’s size when attached to MO.97 The second term ΔEC is the
Coulombic interaction between the electron and hole.
Figure 3.7: A) TA kinetics at the band edge absorption and PL decay of OA-and
MPA-capped CdSe QDs on glass, B) TA spectral components extracted from TA
spectra; inset: steady-state absorption (cyan line) and change in absorption after a
shift of the spectrum by 10 meV (blue line), C) PL decay for CdSe QDs on glass;
inset: PL decay for CdSe QDs with different size attached to NiO, D) hole injection
rate vs driving force of different QDs sizes, and E) schematic illustration of hole
trapping vs hole injection to MO.
Figure 3.7 D shows the hole injection rate dependence on the QD’s size according
to eq. 5. We found that the hole injection rate for CdSe-NiO system is more than an
order of magnitude slower than the electron injection rate for CdSe-ZnO system (paper
I). This can be explained by the hole effective mass being larger than the electron
effective mass and the MO’s permittivity being higher for ZnO than NiO. However,
Exciton dynamics in QDs
29
the most critical factor limiting the hole injection efficiency is the hole trapping which
is strongly competing with the hole injection. We found that growing the shell (1.3 nm
thickness) around the active core will passivate the hole trap states. Consequently, the
hole injection efficiency was enhanced from less than 10% to 50% for core only and
core–shell QDs, respectively.
Exciton dynamics in QDs
30
3333....8 Paper V8 Paper V8 Paper V8 Paper V ““““Energy transfer in CdSeEnergy transfer in CdSeEnergy transfer in CdSeEnergy transfer in CdSe----ZnO NWs ZnO NWs ZnO NWs ZnO NWs
systemsystemsystemsystem”:”:”:”:
One of the important requirements for efficient photoinduced charge separation is the
direct contact between the light absorber and the electron acceptor. However,
multilayers of QDs absorber can boost the solar cell performance as has been reported
for ligand-free QDs.98 Although many models are used to explain the charge collection
from indirectly attached QDs (IA-QDs). In this work we attribute it to the energy
transfer mediated charge collection. Here, the photodynamics in multilayer MPA-
capped CdSe QDs sensitized ZnO NWs with different sensitization time were studied.
Analogous to previous reports,99 in situ steady-state absorption spectroscopy was used
here to quantify the adsorbed amount of QDs on the MO surface. Adsorption can be
described as a combination of a Langmuir-type submonolayer formation and adding
further layers of indirectly attached QDs (aggregation) (see figure 3.8 A). The fraction
of IA-QDs (R) can be calculated as follows:
; = <.=�> ?<.=�> + <.@=,�>A* , (8)
where, <.=�> and <.@=,�> are the concentration of IA-QDs and submonolayer
adsorbed QDs, respectively.
The TA decay kinetics for sensitized ZnO NWs by CdSe QDs show similar decay
components for the electron injection (~10 ps) and CTS dissociation (~100 ps) (paper
I). However, the nanosecond component (~ 3.6 ns) varies with different QDs
sensitization time (see figure 3.8 B). Based on the correlation between the component
amplitude (A3 from the fitting) and the IA-QDs fraction R (calculated from eq. 8) (see
inset of figure 3.8 B) we assign this component to the excitation energy transfer from
the indirectly attached QDs. In addition, the continuous enhancement of the incident
photon-to-electron conversion efficiency indicates that the absorbed photons by IA-
QDs also yield charge carriers. Energy transfer (exciton migration) is the most plausible
mechanism for our system, where the exciton migrates from the IA-QDs to the QDs
adjacent to the MO. Exciton migration from the higher energy (smaller) QDs within
the size distribution of the QDs sample can be confirmed from the steady-state PL
where a pronounced red shift (40 meV) and narrowing of the emission spectrum can
be found in the film of QDs. In contrast to that, no such narrowing occurred in QD
solution (see figure 3.8 C).
Exciton dynamics in QDs
31
Figure 3.8: A) Experimental and theoretical fit of the absorption difference data due
to submonolayer adsorption (DA-QD, red line) and QD aggregation (IA-QD, blue
line), B) TA kinetics of QD sensitized ZnO NWs at different sensitization times;
inset: the fraction of IA-QDs (R, black line, calculated from eq. 8), the amplitude of
TA long-lived component (derived from the three exponential fit, A3), C) steady-
state PL (solid lines) and absorption (dashed lines) of QDs in solution and spin
coated on glass, and D) schematic illustration of the exciton migration from IA-QD
to DA-QD followed by electron injection via CTS model.
Another evidence for the FRET in our sample can be found in TA decay kinetics for
neat QDs on glass, which shows a biexponential character with a conventional radiative
exciton recombination (~ 10 ns) and a faster (~ 660 ps) component corresponding to
the energy transfer from small QDs to larger ones. Finally we can evaluate the energy
transfer time constant from the IA-QDs to the DA-QDs as:
1 'BC = 1 ⟨'⟩ − 1 'DEF⁄⁄⁄ , (9)
where, ⟨'⟩ is the TA lifetime of IA-QDs (3.6 ns), and 'DEF is the exciton lifetime of
QDs without any transfer process. We obtain the energy transfer time constant 'BC
from IA-QDs around 5 ns (see figure 3.8 D). The energy transfer time is significantly
Exciton dynamics in QDs
32
longer than electron injection time. In order to improve this, a well-designed QD
tandem layers with different sizes to provide an ideal spectral overlap for efficient FRET
is indispensable.
Exciton dynamics in QDs
33
3333....9 9 9 9 Paper VIPaper VIPaper VIPaper VI ““““EnergyEnergyEnergyEnergy funneling through multifunneling through multifunneling through multifunneling through multi----sized sized sized sized
QDQDQDQD filmfilmfilmfilmssss”:”:”:”:
After we have proven the exciton migration from IA-QDs to DA-QDs due to the QDs
size distribution in QDs-ZnO NWs system, we turn to study the directed exciton
migration from small to large QDs in more organized multi-sized QD mixtures.
Exciton migration study is also essential for other QD’s applications as light emitters,
lasers and solar cells.100-101 In the development of such devices, QDs are considered as
densely packed to form a thin film with strong absorption and emission. Indeed, FRET
is an important mechanism due to the electronic coupling between the closely packed
QDs.
Here, we report the investigation of FRET dynamics in densely packed multi-sized
CdSe QDs (we used three different QDs: QDs-A, 2.3 nm, QDs-B, 3.7 nm, and QDs-
C, 6.7 nm) based on TA spectroscopy and theoretical modeling. Firstly, steady-state
PL spectroscopy for multi-sized CdSe QDs film (A+B) shows a typical indication of
FRET: a significant increase of the red emission on the expense of the blue emission
due to exciton migration from small QDs to large QDs (see figure 3.9 A). However,
steady-state PL spectra do not provide a full proof of FRET, therefore, we used TA
measurements to prove the FRET presence and to reveal its time scale. TA spectra at
different delays (t) for singly-sized QDs (ΔαA(t), ΔαB(t), ΔαC(t)) and for different
combinations of QDs (A+B, A+C, B+C) (ΔαA+B(t)) at the same delays were recorded,
then fitted using the sum of TA spectra for singly-sized QDs at the same delays:
∆ GH!�I� = JG�I�∆ G�I� + J!�I�∆ !�I�, (10)
The ratio of single-color spectrum (kA(t)/kA(0) for QD-A, and kB(t)/kB(0) for QD-B)
corresponds to the FRET-related change of the excited state population in A and B
relative to their initial population. This ratio gives us valuable information about FRET
dynamics, if this ratio stays the same at different delays for A and B (for example, A+B
mixture in solution) this means no FRET dynamic within A and B mixture (see figure
3.9 B and C). On contrary, for the same mixture in the film form, a significant decrease
of the ratio of QD-A accompanied by increase of the ratio of QD-B with similar
kinetics can be observed. The same effect takes place for the other pair combinations
(see figure 3.9 D). For all possible QD pair combinations, the FRET times were
estimated based on the analysis to be 1-3 ns for different combinations.
Exciton dynamics in QDs
34
Figure 3.9: A) Steady-state PL spectra of QD-A and QD-B individually and a
mixture of QDs-(A+B) on glass, B) TA spectra of QD-A, QD-B, and QD-C
individually in solution and a mixture of QDs-(A+B+C) in solution as well, C),ratio
of single-color spectrum as a function of pump–probe delay times of QDs-(A+B+C)
in solution, and D) ratio of single-color spectrum as a function of pump–probe delay
times of QDs with different combinations on glass.
The estimated values did not follow the (1/;EGL ) dependence according to the
standard FRET rate expression (eq. 11).
JBC = 1 'BC⁄ = ;EGL MN ���
ℏ PE� PG
�Q�R�* , (11)
where, RDA is the donor-acceptor distance, μD and μA are the donor and acceptor dipole
moments, respectively, K2 refers to the orientation factor of the dipole–dipole
interaction, n is the medium’s refractive index, and R is the spectral overlap between
the normalized donor emission and acceptor absorption line shapes. Apparently the
simple dipole–dipole description of FRET is not sufficient because of the distance
between donor and acceptor is smaller than the QD dimensions.
We took into account the dipole moment distribution over the whole QD using
Bessel function to describe the exciton wavefunction density in spherical QDs. The
Measured data
Fitting result
QDs-A
QDs-B
QDs-C
500 550 600 650 700-0.025
-0.020
-0.015
-0.010
-0.005
0.000
1 10 100 1000 100000.0
0.5
1.0
1.5
2.0
∆∆ ∆∆ A
bs.
Wavelength (nm)
QDs-A QDs-B QDs-C
Rati
o o
f si
ngle
colo
r
spec
tru
m
Delay (ps)
BBBB
CCCC0.0
0.5
1.0
1.5
2.0
0.0
0.5
1.0
1.5
1 10 100 1000 100000.0
0.5
1.0
1.5
Rati
o t
o s
ingle
colo
r s
pectr
um
QDs-B
1.5 ns
QDs-A
2 ns
QDs-B
QDs-C
QDs-A
Delay (ps)
QDs-C1.5 ns
DDDD500 525 550 575 600 625 650 675
0.0
5.0x106
1.0x107
1.5x107
2.0x107
QDs-A
QDs-B
PL
in
ten
sity
fo
r s
ing
le c
olo
r
Wavelength (nm)
0
1x104
2x104
3x104
4x104
5x104
6x104
PL
in
ten
sity
fo
r m
ixed
co
lors
QDs (A+B) on glassAAAA
Exciton dynamics in QDs
35
function drops quickly with increasing the distance from the QD’s center, but still the
dipole distribution influences the interaction of two close QDs (see figure 3.10 A, lower
inset). In order to incorporate the dipole distribution into the FRET theory, we have
modified the “1 ;EGL⁄ ” term (distance term). Namely, we numerically integrate the
dipole–dipole interaction over the volume of donor and acceptor. Our calculations
show that for distances less than 10 nm between donor and acceptor (here, for our
combinations the center-to-center distances range 3-5 nm) the point–dipole
underestimates the resulting FRET rate but for larger distances the point–dipole
approximation is sufficient (see figure 3.10 A). For closely staked QDs, the correction
of the distance term based on Bessel distribution can be more than 50% (see figure
3.10 A, upper inset).
In reality, the QD–QD distances given by the film morphology play also an
important role in FRET rate. In the previous reports often the ideally stacked QD layers
were used to calculate the FRET rate. We have used atomic force microscopy (AFM)
and found a big deviation from the ideal model due to the fabrication procedure. The
QDs tend to aggregate into clusters after ligand exchange.102 We compared our
experimental FRET rates to the calculated rates based on our modifications. As the
distance between QD and the closest neighbor is not a single value, but a distribution,
our calculations result in a distribution of FRET rates around mean value on the
nanosecond time scale. For all the combinations, the mean FRET rates agree with the
FRET rates obtained experimentally (see figure 3.10 B).
Finally, we study the directed energy funneling between tandem layers of QDs with
different sizes. We use steady-state PL for different combinations of QD monolayers
where QD-C is used as the exciton final acceptor and QD-A is the donor. In between
the A and C monolayers we deposit one or two layer(s) of QD-B. In both cases (A+B+C)
and (A+2B+C) (see figure 3.10 C), about 90% of the excitons from QD-A is taken off
due to fast FRET compared to the exciton life time in QD-A. The extra QD-B layer
did not affect the exciton migration from QD-A but it decreases the number of excitons
transferred to the QD-C by 20%. This pronounced effect of the extra QD-B layer on
the exciton migration stimulated us to extract the exciton diffusion length LD for B-C
QDs combination with different number of QD-B layers. We estimate the diffusion
length to be 9.0 nm. For a single layer of QD-B, 95% of excitons transferred to QD-
C (FRET lifetime 3.0 ns, exciton lifetime 28 ns). On the other hand, for many QD-B
Exciton dynamics in QDs
36
layers (LD ~ two layers of QD-B), many excitons cannot reach B/C interface and
recombine before the final destination (QD-C) (see figure 3.10 D).
Figure 3.10: A) Distance term of FRET for δ-function approximation (1 ;EGL⁄ ,
black points) and Bessel function model (red points); lower inset: the corresponding
density of dipole moments in the models; upper inset: correction ratio obtained via
Bessel function, B) left panels: experimental ratio of the excitons transferred to donor
(blue lines) compared to the theoretical prediction (red lines), and right panels:
distribution of FRET lifetimes for each pair combination, C) PL spectra of ordered
QDs films, and D)PL ratio between QD-B on glass and QD-B with top layer of
quencher (QD-C) as a function of the number of QD-B layers in order to extract
the exciton diffusion length LD.
500 550 600 650 700 7500
2000
4000
6000
8000
10000
12000
C
2×B
PL
In
ten
sity
Wavelength (nm)
C
2×B
A
A only
0 5 10 15 20 25 30 350.0
0.2
0.4
0.6
0.8
1~5 layer
Number of QD layers
PL
rati
o (
I qu
en
ch
ed/I
non
qu
ench
ed)
Length (nm)
QDs-B
Glass
QDs-C1 layer
θ
LD= 9 nm
4.7 nm
QD B
1 2 3 4 5 6 7 8
DDDDCCCC
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10 1001E-12
1E-10
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Dis
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erm
(n
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)
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δδδδ-function
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0 5 10 15
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o
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sity
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0.00
0.01
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BBBB
Photoinduced dynamics in core–shell QDs
37
Chapter Chapter Chapter Chapter 4444: : : : Photoinduced dynamics in Photoinduced dynamics in Photoinduced dynamics in Photoinduced dynamics in corecorecorecore––––shell QDsshell QDsshell QDsshell QDs
4.1 Motivation4.1 Motivation4.1 Motivation4.1 Motivation::::
Understanding the fundamental science and the synthetic methodologies of the nano-
heterostructures provides a wealth of new materials, devices, and applications103
Nano-heterostructure crystals (such as, semiconductor-core–semiconductor-shell
QDs) feature highly diverse physical and chemical properties, as we will discuss later.103
Great flexibility in tuning the optical and electronic properties can be achieved by
integrating the nanomaterials into the nano-heterostructures (for example, core–shell
quantum dots, CSQDs). Such structures often lead to significantly improved device
performance. Since 1990, CSQDs have been actively investigated in order to overcome
the surface photodegradation of core-only nanocrystals.103 Coating a semiconductor
QDs (CdSe QDs) by another semiconductor (such as ZnS) can enhance the chemical,
thermal, and photochemical stability compared to the neat QDs. In the CSQDs, the
semiconductor shell is grown on the semiconductor core. The shell improves the
surface passivation of the core by separating the surface dangling bonds from the core
material with an energy barrier in-between. Optical and electronic properties can be
tuned easily by engineering the band alignment between core and shell materials and
consequently it opens the door for these materials to be useful to a wide variety of
fields.104-105
4.2 4.2 4.2 4.2 Classification of coreClassification of coreClassification of coreClassification of core––––shell QDs:shell QDs:shell QDs:shell QDs:
Depending on the VB and CB of the core and shell semiconductors, CSQDs can be
classified into three main categories. Type I CSQDs, reverse type I CSQDs, and type
II CSQDs.
In the type I CSQDs, a shell with a wider band gap than the core is grown around
the core, aiming to improve the properties of the active core (see figure 4.1). For
instance, the shell can passivate the surface traps (usually induced by dangling bonds)
on the core’s surface with energy barriers. This leads to the enhancement of the PL QY
Photoinduced dynamics in core–shell QDs
38
by reducing the non-radiative recombination from the traps (e.g., CdSe–ZnS CSQDs).
CSQDs usually show red-shifted excitonic peaks compared with the core materials due
to the partial leakage of the exciton wavefunctions from the core into the shell.106
Figure 4.1: Different types of CSQDs compare to neat core depending on the band
gaps energy of both core and shell materials.
In reverse type I CSQDs, a wider band gap core is coated with a narrower band gap
shell. Thus, the carriers are partially or completely induced and confined in the shell
which improves the charge extraction and injection (e.g., CdS–CdSe and ZnSe–CdSe).
The excitonic peak can be red-shifted by increasing the shell thickness. In order to
improve the photostability and the PL QY properties, growing a second shell with
wider band gap than the first one (core–shell–shell structure, CSS) is needed.106
In the type II CSQDs, either the CBM or the VBM of the core is located within the
band gap of the shell. Consequently, the resulted effective band gap is always smaller
than each one of the constituting core and shell materials (see figure 4.1). This
alignment leads to spatial separation of the electrons and holes into the core or the shell
depending on their band alignment. Manipulating the shell thickness of this type leads
to tuning the emission color which is of the main interest in such system (e.g., CdTe–
CdSe and CdSe–ZnTe).106 The PL lifetime for this type of CSQDs is much longer
compared to type I CSQDs due to the lower wavefunctions overlap of the electrons
and the holes. Again growing a second shell with wider band gap (CSS) is needed here
to improve the photostability and the PL QY. Quasi-type II CSQDs denote a structure,
Photoinduced dynamics in core–shell QDs
39
where one of the carriers is delocalized over the CSQD volume and the other carrier is
mainly confined within the core only.103
Among all above-mentioned types of CSQDs, the transition from the core to the
shell materials is sharp, resulting in step-like band alignment.107 In such case,
continuously growth of shell in type I CSQDs would greatly reduce the PL QY.107 This
is due to the lattice mismatch between the core and the shell layers, the nonuniform
growth of the shell, and the formation of grain boundaries between small clusters in
the shell layer.20, 64 The lattice mismatch refers to the situation where two materials
featuring different lattice constants are brought together with interface between them.
All these effects will induce defects acting as carrier traps and hence reducing the PL
QY.
On the contrary to step-like CSQDs, one can also form so-called the gradient type I the gradient type I the gradient type I the gradient type I
CSQDsCSQDsCSQDsCSQDs (see figure 4.1), where the composition changes smoothly in the radial
direction and resulting in a gradual band change from the core to the shell. In this case,
the above-mentioned shell induced defects can be minimized, and the PL QY can be
enhanced. In particular, in gradient CSQDs the soft confinement of electrons and holes
can reduce the unwanted AugR rate compared with step-like CSQDs which have sharp
steps of potential change.29, 83, 108 In the following section we will explain the general
aspects of designing the gradient type I CSQDs (Cd1-xZnxSe1-ySy) which are used in this
thesis in order to improve the core properties for solar cell applications.
4444....3333 Important aspects for preparing the gradient type I Important aspects for preparing the gradient type I Important aspects for preparing the gradient type I Important aspects for preparing the gradient type I CSCSCSCSQDs:QDs:QDs:QDs:
In the following section we will discuss the preparation of gradient Cd1-xZnxSe1-ySy
CSQDs of type I in details. In general for step-like CSQDs, cores with a known
diameter were used as a seed to grow the shell around in a two-steps synthesis procedure
(core synthesis followed by purification process and then growing the shell over the
core). This two-steps synthesis route might create interfacial defects between core and
shell due to the lattice mismatch. However, in order to prepare the gradient type I
CSQDs, we employed the single-step synthesis procedure where the core and shell
materials are introduced at the same time during the growth. The gradient structure is
greatly determined by the following important factors during the synthesis: the
composition of the core and shell materials, the shell precursor’s materials, the chemical
Photoinduced dynamics in core–shell QDs
40
reactivity of the different precursors, the reaction temperature, and the shell thickness
control.
We will start by choosing the core and shell materials, where the lattice mismatch
between them plays an important role. For CSQDs, the smaller the lattice mismatch
the lower the density of core–shell interface defect states would occur. For the type I
step–like CSQDs (sharp core–shell interface), the PL QY is increasing with the shell
thickness up to ~ 0.7 nm (~ 2.4 monolayers) and then is decreasing due to the formed
defects due to the lattice mismatch between the core (CdSe) and the shell (ZnS).107, 109-
110 On the other hand, the PL QY of the gradient CSQDs increases gradually with the
shell thickness up to ~ 1.6 nm due to the successive relaxation of the core–shell interface
strain via chemical composition gradient.20 For the thicker shell (> 1.6 nm), the QY
does not increase any more due to lattice imperfections within the shell.109-110
The selection of the shell precursor’s materials is another important issue to be taken
into account to avoid side reactions and unwanted products. In addition, some
precursors require special precautions especially when they are highly toxic and/or
pyrophoric chemicals. For instance ZnS, is one of the most used shell materials for
numerous II–VI and III–V semiconductor NCs.106 The ZnS shell can be grown based
on using diethylzinc and hexamethyldisilathiane as Zn and S precursors, respectively.
However, these two chemicals are pyrophoric and toxic, respectively. Therefore,
alternative precursors were employed in our gradient CSQDs - namely zinc
carboxylates and elemental sulfur which are more suitable for large scale CSQDs
production.106
In the single-step synthesis of the gradient Cd1-xZnxSe1-ySy QDs, both Cd2+ and Zn2+
add together with oleic acid in presence of non-coordinating solvent (namely, 1-
octadecene). Then after the formation of Cd-oleate and Zn-oleate, a mixture of the
anionic precursors (Se2- and S2-) in TOP is quickly injected into the cationic mixture.
Thus, the chemical reactivity difference between the cationic (Cd2+ and Zn2+) and the
anionic (Se2- and S2-), indeed, is very important. In our CSQDs, even if the initial
concentration of the Zn2+ cation was 10 times higher than Cd2+ (in precursor solution),
after 5 sec of the reaction the amount of reacted Cd2+ was 20 times higher than Zn2+
(determined using EDX, see the following sections). This shows that the chemical
reactivity of Cd2+ is much higher than Zn2+. In the same manner, the chemical reactivity
of Se2- is much higher than S2-. Due to both the initial concentration difference and the
chemical reactivity difference between Cd2+(Se2-) and Zn2+(S2-), the gradient shell is
Photoinduced dynamics in core–shell QDs
41
formed after 5 sec when the concentrations of Cd2+ and Se2- decreased drastically while
the concentrations of Zn2+ and S are still high to form the gradient shell.
Choosing the proper injection and growth temperatures is very important for
successful CSQDs synthesis. In order to avoid the shell material nucleation, both
injection and growth temperatures were chosen to be below the ZnS nucleation
temperature. Finally, controlling the shell thickness is very important and it was the
keystone of our study. We controlled the shell thickness by cooling the reaction mixture
suddenly after the desired growth time by using an ice bath.
4444....4444 Characterization of type I Characterization of type I Characterization of type I Characterization of type I gradient gradient gradient gradient CdCdCdCd1111----xxxxZnZnZnZnxxxxSeSeSeSe1111----yyyySSSSyyyy CSQDsCSQDsCSQDsCSQDs::::
Most of the basic techniques used to characterize the neat core QDs can be used also
for the CSQDs characterization. In the following sections we will present the different
techniques used to characterize the gradient CSQDs. Starting with steady-state optical
spectroscopy techniques and high resolution transmission electron microscopy (HR-
TEM) in order to determine the core size and to estimate the shell thickness for
different CSQDs. Then we conducted X-ray based spectroscopies in order to
characterize the crystalline and composition such as, X-ray diffraction (XRD) and
energy-dispersive X-ray spectroscopy (EDX).
4.4.1 Core size determination and shell thickness estimation for
gradient CSQDs:
The dimensions of our CSQDs (core sizes and shell thickness) were obtained via HR-
TEM. The results were verified by the steady-state optical spectroscopies using the
known size dependences of the absorption spectra (see figure 4.2 A). The HR-TEM
images are show in figure 4.2 B. By careful analysis of the CSQDs HR-TEM images
and subtracting the core size (3.0 nm) we determined the shell thickness for different
growth time to be 0.6, 1.3, 1.6, 1.9, and 2.3 nm for 1, 3, 5, 10, and 15 min. Figure
4.2 A, presents the steady-state UV-Vis absorption and PL for core (sample (i)) and
CSQDs with different thicknesses (ii, iii, and iv for 0.6, 1.3, and 2.3 nm shell
thicknesses, respectively). The excitonic peak is well resolved for the core which can be
used to estimate the QD size according to the previous reports.111 It revealed the size of
3.0 nm for our core QDs consistent with the TEM observations. Such excitonic peaks
Photoinduced dynamics in core–shell QDs
42
can also be shown in the CSQDs with different shell thicknesses up to ~ 1.3 nm (see
figure 4.2 A, red lines). For QDs with the thickest shell (> 1.3 nm), there is no
pronounced excitonic peak (see figure 4.1 A) due to the carrier confinement reduction
by extension of the electron and hole wavefunctions into the shell material.112 For all
the samples, the PL spectrum consists of a single band (FWHM < 33 nm) indicating
relatively narrow QD size distribution (see figure 4.2 A, black lines).
Figure 4.2: A) Steady-state UV-Vis (red lines) and PL (black lines) of the core (i) and
CSQDs of different shell thicknesses (ii, iii, and iv for 0.6, 1.3, and 2.3 nm shell
thicknesses, respectively), B) HR-TEM for the same samples as A).
4.4.2 Structural characterization of gradient CSQDs”:
In order to better understand the optical properties of our gradient CSQDs, one needs
to get insight into the exact structures of the QDs. Particularly, we have studied the
chemical composition and crystalline structures for our QDs with different shell
thickness. We employed EDX and synchrotron-based XRD to estimate the
composition and the crystal structure. Figure 4.3 A shows the XRD patterns for the
neat core and the gradient Cd1-xZnxSe1-ySy CSQDs of different shell thicknesses. We
call the pure CdSe QDs as neat cores, and we use them as references. The neat core is
compared to CSQDs with six different shell thicknesses, ∼“0”, 0.6 1.3, 1.6, 1.9, and
2.3 nm obtained by growth times of 5 s, 1, 3, 5, 10 and 15 min, respectively. For the
CSQDs of 5 s growth time, it has intermediate properties between the neat core and
the CSQDs with a 0.6 nm shell thickness, therefore we call it “0” nm CSQDs. We also
show the XRD spectra of the CdSe and ZnS zinc blende structures. The XRD patterns
of our CSQDs were analyzed in terms of these two structures where the core is more
Photoinduced dynamics in core–shell QDs
43
like CdSe phase and the thickest shell is approaching the ZnS phase. The fitting results
provide the lattice parameters for both phases, where one lattice constant is close to the
core (CdSe) and the other is close to the shell (ZnS) (see figure 4.3 B). A clear decrease
in the core unit cell constant as the shell grows up to 1.3 nm is observed. This can be
attributed to the compressive strain of the shell on the core. For CSQDs with thicker
shell thickness than 1.3 nm, the strain in the core is released. The reason behind this
phenomena is not clear, but it may relate to the defect sites which are induced by the
growth of the shell.
Figure 4.3: A) XRD patterns of neat core and CSQDs of different shell thicknesses
compared to zinc blende CdSe113 and ZnS114, B) lattice constants of CdSe core
(black) and ZnS shell (red) as a function of the shell thickness, the gray and red areas
present the lattice constants of bulk CdSe and ZnS, respectively, and C) EDX
average element ratio for different growth time for Cd/(Cd+Zn), dark yellow line
and Se/(Se+S), orange line.
EDX spectra were used to evaluate the chemical composition for the different
CSQDs (see figure 4.3 C). EDX revealed that due to the difference in chemical
reactivity between Cd (Se) precursor and Zn (S) precursor, at the early stage of the
reaction (5 sec) Cd-rich (Cd1-xZnxSe1-ySy) core (small band gap) is formed first, followed
0.6 nm
2.3 nm
1.9 nm
1.6 nm
1.3 nm
"0" nm
Inte
nsi
ty
Bare Core
10 20 30 40 50
2θθθθ
422
331
400
31
1220
200
111
Bulk (Zinc-Blende) CdSe
Bulk (Zinc-blende) ZnS
331
400
3112
20
200
111
Core "0" 0.6 1.3 1.6 1.9 2.3 5.2
5.4
5.6
5.8
6.0
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Shell
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ell
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Shell thickness (nm)
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0 150 300 450 600 750 9000.1
0.2
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0.5
0.6
0.7
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Average e
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Growth time (sec)
"0" nm
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1.6 nm shell thickness
1.9 nm shell thickness
2.3 nm shell thickness
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Photoinduced dynamics in core–shell QDs
44
by an alloyed shell over the core. Later the Zn-rich (ZnS) shell (wide band gap) will
externally coat the core.20
Photoinduced dynamics in core–shell QDs
45
4444....5555 Paper VIIPaper VIIPaper VIIPaper VII “Electron “Electron “Electron “Electron injection from injection from injection from injection from gradient gradient gradient gradient
CdCdCdCd1111----xxxxZnZnZnZnxxxxSeSeSeSe1111----yyyySSSSyyyy CSQDs to MO”CSQDs to MO”CSQDs to MO”CSQDs to MO”::::
The overall device efficiency of a QD-sensitized solar cells is determined by many
factors such as light harvesting, charge separation, and charge transport.110 If one
utilizes CSQDs in solar cells, the enhanced photostability and the reduction of charge
recombination by surface trapping is expected, but the existence of shell may also
hinder the charge transfer process from QDs compared to neat QDs. Thus those effects
should be overviewed comprehensively during the evaluation of CSQDs in solar cell
applications. In this paper we studied the dependence of both the electron injection
and the trap passivation on the shell thickness in gradient Cd1-xZnxSe1-ySy CSQDs/ZnO
NPs system. We managed to estimate an optimal condition for the best overall electron
collection efficiency.
Figure 4.4: A) TA kinetics of gradient CSQDs of different shell thicknesses (ii, iii,
and iv for 0.6, 1.3, and 2.3 nm shell thicknesses, respectively) compared to core QDs
(i) (red circles are from experiment and red lines are fitted data for QDs in solution;
black circles and black lines represent the experimental and fitted data for QDs
attached to ZnO NPs), B) mean decay rate dependence on the shell thickness for
QDs in solution (red), QDs attached to ZnO NPs (black), and reported values for
step-like CSQDs of the same materials (blue)110, C) electron injection efficiency and
PL QY as a function of shell thickness, and D) energetic scheme for electron
tunneling through the shell followed by electron injection to ZnO NPs for step-like
CSQDs (upper) and gradient CSQDs (lower).
Photoinduced dynamics in core–shell QDs
46
TA decay was used to study the electron dynamics in QDs, as we discussed
previously. The TA kinetics of unattached CSQDs were fitted using a biexponential
function resulting in a minor subnanosecond and a dominant nanosecond components
(A1 = 20–45%, τ1 = 0.1–0.3 ns; A2 = 55–80%, τ2 = 12–18 ns) (see figure 4.4 A, red
lines). The observed multiexponential decay has the same character as previously
reported decays of single exciton in CdSe QDs affected by fluctuating rates of
nonradiative processes (QDs charging, change in surroundings, etc.).115-116 The decay
of neat CSQDs was then compared to the CSQD-MO case. Clearly, the attachment
of the QDs to the MO affects the TA decay kinetics due to the electron injection from
QDs to MO (see figure 4.4 A, black lines). The experimental data could not be
reproduced by a simple multi-exponential function and therefore we employed a
stretched-exponential function:
∆T�I� = ∆T�0� × exp Z−?�I '[B⁄ �A!\, (12)
The function has been previously used to describe the dynamics in disordered
nanomaterials and electron injection in QD-MO systems.117-118 Here, '[B is the decay
time and B is the dispersion factor (0 < B < 1) which reflects the disorder degree for the
studied system. It should be noted that we use B instead of commonly used β to avoid
confusion with the later used β factor. The thicker the shell, the more the disorder in
the system for gradient CSQDs can occur due to different composition and thickness
might vary from QD to another. By using the fitting data, we calculated the mean
lifetime of the stretched-exponential function:
⟨'⟩9[DE]^_,( = �'[B `⁄ � ∗ Γ�1 `⁄ �, (13)
where c stands for the Gamma function.
The calculated ⟨'⟩9[DE]^_,( shows a clear dependence on the shell thickness
ranging from 6 ps for core to 15 ns for 2.3 shell thickness. Then the electron injection
rate was calculated for each shell thickness by comparing ⟨'⟩9[DE]^_,( and ⟨'⟩9[DE]
as follows:
JBC�d� = ?1 ⟨'⟩9[DE]^_,(⁄ A − ?1 ⟨'⟩9[DE]⁄ A, 14
Due to the uncertainty in stretched-exponential fit, the TA mean decay time of the
thickest shell layers becomes slower after the attachment. Therefore, we consider the
injection rate for 1.9 and 2.3 nm shell thickness as ~ 0. In Figure 4.4 B we compare
Photoinduced dynamics in core–shell QDs
47
the mean decay rates as a function of the shell thickness for reported step-like CdSe–
ZnS CSQDs110 (blue line) and for the gradient Cd1-xZnxSe1-ySy CSQDs (black). Both
CSQD structures follow the expected exponential dependence eq. 15. This dependence
is a result of the distance that electron has to tunnel through the shell in order to be
injected to ZnO NPs.
JBC�d� ∝ ?f^ghA, (15)
The typical i values for step-like CSQDs are reported to be 0.33-0.35 Å-1 depending
on the shell material.110 However, for the gradient CSQDs a larger i value (0.51±0.05
Å-1) was obtained. In the step-like CSQDs as the shell thickness increases, only the
energy barrier width increases (see figure 4.4 D, upper panel). In case of the gradient
CSQDs both the barriers’ width and height increase as the shell thickness increase (see
figure 4.4 D, lower panel) which explains the stronger shell thickness dependence of
the injection rates.
For the solar cell applications, the electron injection efficiency is the important
parameter. We can calculate the efficiency based on the experimental data as follows:
jk,l = JBC �JBC + J+�⁄ , (16)
Even if the electron injection rate drops quickly with the shell thickness, the electron
injection efficiency stays almost unaffected for the shell thickness up to 1.2 nm due to
the long recombination lifetimes in QDs (see figure 4.4 C, black line). Moreover we
have studied surface passivation of QDs by measuring the PL QY for each shell
thickness (unattached QDs). For 1.2 nm shell thickness the PL QY is about two times
higher than the core QDs (see figure 4.4 C, blue line). By combining the information
about electron injection and surface passivation we obtain the optimal shell thickness
~ 1.2 nm, which acts as a shield around the core against surface degradation and surface
trap states, at the same time keeping high electron injection efficiency > 80%.
Photoinduced dynamics in core–shell QDs
48
4444....6666 Paper Paper Paper Paper VIIIVIIIVIIIVIII “hole trapping “hole trapping “hole trapping “hole trapping vsvsvsvs.... quantum dot quantum dot quantum dot quantum dot
sensitized solar cell performance”sensitized solar cell performance”sensitized solar cell performance”sensitized solar cell performance”::::
In general, solar cell efficiency depends on the behavior of both photoexcited electrons
and holes.119 In this paper, we confirm the role of the shell thickness in the real CSQDs
solar cell device within certain shell thickness range. We prove that this happens by
decreasing the surface defect states which acts as hole traps (see paper IV). Moreover,
we combined our knowledge about the electron (paper VII) and hole behavior to
explain the dependence of solar cell efficiency on QD shell thickness.121
Figure 4.5: A) PL decay of MPA-CSQDs with different shell thickness compared to
MPA-CdSe QDs up to 1.5 ns, B) PL decay of the early time (up to 75 ps) for the
neat core and different CSQDs, C) I-V characteristics for the core CdSe QDs
compared to the CSQDs with different shell thickness (all are compared to the dark
current, gray area), D) electron collection efficiency (e collection eff., blue line),
electron injection efficiency (e Inj. eff., black line, according to ref.120), hole
scavenging efficiency (h scavenging eff., red line), and combined efficiency (pink
line) as a function of shell thickness, and E) scheme for electron and hole tunneling
through the shell followed injection to MO and S2-/SX2- electrolyte, respectively.
Linker exchange is necessary to attach the QDs to the MO. However, the exchange
introduces numerous surface defects acting as trapping centers resulting in drastic drop
in PL QY for neat core after the linker exchange.57, 122 We have studied the effect of
linker exchange on the CSQDs, where the effect of traps is diminished by the shell
Photoinduced dynamics in core–shell QDs
49
layer. Figures 4.5 A and B represent the PL decay kinetics for CSQDs before
attachment to MO. By using the multiexponential function to fit the decay of the
studied QDs, we revealed two fast decay components (9–18 ps and ~ 120 ps) for the
neat core, “0” nm and 0.6 nm shell thickness samples. These fast components are
related to defect states of different origins.56-57 Independent of the origin of these traps,
the fast components were gradually diminished with increasing the shell thickness and
they have been completely vanished by the 1.3 nm thick shell, when the QD’s surface
is almost completely passivated.
In order to study the passivation effect on real device performance, we fabricated
several sets of solar cell devices. Figure 4.5 C shows the current–voltage (I–V)
characteristics of the gradient CSQDs-based devices compared to neat core QDs-based
device. The measurements were done under a simulated AM1.0G solar irradiation
(light intensity of 100 mW/cm2). The solar cell efficiency increases with QD shell
thickness reaching the maximum value at 1.3 nm shell thickness and then starts to
decrease. Furthermore, we have evaluated the cells’ performance by calculating the
electron collection efficiency (ECE). ECE is the ratio between the extracted electrons
out of the device and the number of photons absorbed by the device:
jB9 = 8mn�-,]/n=)]-�)h o�-n-,]/n , (17)
The electron collection efficiency increases with the shell thickness reaching 6% for
1.3 nm shell thickness. Then for thicker shell the electron collection efficiency decreases
again. We can compare the observed values with electron and hole injection efficiencies.
For the thin shell thickness the electron injection efficiency (see paper VII) is very high
and drops exponentially with increasing the shell thickness as the core/MO distance
increase. Consequently, the electron collection efficiency drops with increasing the shell
thickness. Thus the low value of jB9 for the thin shell is related to the hole trapping
process.
In order to quantify the hole collection efficiency we have assumed that the radiative
dipole of the excited electron–hole pair where the hole is trapped is negligible. We
managed to quantify also the hole collection efficiency (untrapped holes). These
untrapped holes can be efficiently scavenged by the electrolyte, thereby j� is the hole
collection efficiency. We quantify j� by evaluating the proportion of the untrapped
holes as a ratio of the PL intensity at the 1.5 ns delay and PL amplitude in the PL
dynamics in Figure 4.5 D as follows:
Photoinduced dynamics in core–shell QDs
50
j� = pqrs.t uv^pwx�y�xzpqr"^pwx�y�xz
, (18)
where, It=1.5 ns is the PL intensity at 1.5 ns, It=0 is the PL amplitude, and Iprezero is the
intensity before time zero which is due to long PL lifetime (~ tens of ns) compare to
the time window. The time 1.5 ns was chosen as a delay long enough to allow complete
hole trapping yet fast enough that exciton recombination does not play a prominent
role. Total charge collection efficiency is the product of electron and hole injection
efficiencies. It agrees very well with the charge collection efficiency obtained from real
solar cell performance measurements (see figure 4.5 D pink line).
Figure 4.5 D summarizes the photodynamics of the gradient CSQDs in real solar
cell device. Here, the neat CdSe QDs without any shell protection feature high electron
injection efficiency (~100%), while most of the holes (> 80%) cannot be collected due
to the hole trapping process. Thus, the trapped holes are not able to be injected to the
electrolyte probably due to insufficient driving force.57 Passivation of the hole traps
using core–shell structures provides an efficient way to enhance the hole collection.
However, shell is also an energy barrier preventing the electron/hole transfer from the
core. Fortunately, Cd1-xZnxSe1-ySy CSQDs with shell thickness up to 1.3 nm can offer
electron injection efficiency up to 80% and at the same time an efficient passivation
for the hole traps. Also, based on the charge carrier photodynamics we calculated the
charge carrier (electron and hole) injection efficiency and used these efficiencies to
predict the charge collection efficiency. The result is in good agreement with the
obtained values (see figure 4.5 D pink line). Figure 4.5 E illustrates the 1.3 nm shell
thickness device with efficient electron and hole injection.
Conclusions and future work
51
Chapter 5:Chapter 5:Chapter 5:Chapter 5: ConclusionsConclusionsConclusionsConclusions and future and future and future and future workworkworkwork
5.1 Conclusions5.1 Conclusions5.1 Conclusions5.1 Conclusions::::
We believe that an important way to improve the application of QDs in solar cell fields,
is to understand the photoinduced dynamics in such systems. The thesis presents the
fundamental science of the ultrafast photoinduced dynamics in CdSe QDs and
gradient Cd1-xZnxSe1-ySy CSQDs. We covered, almost all, the possible carrier’s
dynamics (electron injection, hole trapping/injection, and exciton migration) in these
QDs between the folds of this thesis.
We observed directly, by using the combination of time-resolved absorption and
THz spectroscopy, the ultrafast electron injection from neat CdSe QDs to the n-type
MO namely, ZnO NWs. We proved that the electron injection-driving force
dependence can be described by the well-known Marcus theory for charge transfer.
Such ultrafast electron injection process encouraged us to study the multiple electron
injection under high excitation intensity condition. Multiple electron transfer is a
prerequisite for successful utilization of multiple exciton generation for photovoltaics.
We observed a competition between the electron injection process and AugR
(multiexcitons quenching) process under these conditions. Indeed, we found that the
second electron injection is possible, however the multiple exciton harvesting can be
efficient only within a narrow range of QD sizes for the CdSe-MPA/ZnO NWs system.
Defect and/or surface states play an important role in the charge collection in QDs
solar cells. We determined the lifetime of the deep trapped holes for OA capped-CdSe
QDs to be around few tens of microsecond at room temperature. Moreover, we
revealed that at least two different types of surface states (traps) contribute to the surface
PL. Excitons with energy higher than the band gap have higher chance to get trapped
by surface states than the band gap excitons. When utilizing QDs in p-type solar cells,
we managed to distinguish between the hole trapping and hole injection processes in
QDs/NiO mesoporous film system. We found that the hole trapping process is more
dominant especially after linker exchange process. Passivating of the hole trap states
using core–shell structure is found to enhance the hole injection efficiency from < 10%
Conclusions and future work
52
to 50%. Similar to electron injection process, hole injection from CdSe QDs to NiO
followed the Marcus theory for charge transfer.
Besides the charge transfer, exciton migration may also occur in QD solar cell system.
Understanding the Förster resonance energy transfer (FRET) in QDs system is
therefore of fundamental and technological significance. In conventional QDs-
sensitized solar cell structures, we found the energy transfer between QDs in QD-
MPA/ZnO NWs system is ~ 5 ns. We also studied the FRET in densely packed multi-
sized CdSe QDs films. We revealed that point–dipole approximation for FRET is
insufficient in this case. We suggested to use a model taking into account the
distribution of the electronic transition densities in the QDs and using the real film
morphology (center-to-center distance) revealed by AFM images. By taking these two
aspects into account we were able to fully describe the FRET kinetics in our system.
Conventional neat core QDs usually suffer from surface defects as charge traps in
solar cell application. This can be well solved by using core-shell structure to passivate
the surface traps and reduce charge recombination. Here we investigate the
photodynamic of gradient Cd1-xZnxSe1-ySy core–shell QDs in solar cells. Growing the
shell in the gradient way reduces the interfacial defects and also the unwanted AugR
compared with step-like counterparts. In this context, we were interested to study the
electron photoinduced injection from the gradient Cd1-xZnxSe1-ySy CSQDs to n-type
ZnO NPs. We observed the typical exponential injection rate dependence on the shell
thickness (β = 0.51 Å-1). Compared to step-like CSQDs (β = 0.35 Å-1), gradient CSQDs
have stronger electron injection rate dependence on the shell thickness. We attributed
this enhanced dependence to the gradient feature where both the barriers’ width and
height change as the shell thickness increase. Although the shell materials always serve
as barriers against the charge injection, we found that ~ 1.2 nm shell thickness still
offers ~ 80% electron injection efficiency from the CSQDs to ZnO NPs and at the
same time keeps high PL QY (~ 70%) which reflects high surface passivation.
Combining our findings regarding the hole trapping process and the performance of
CSQDs-based solar cells, both in respect to the shell thickness. We found that the hole
traps are almost diminished for ~1.3 nm shell thickness. As a results, solar cell based on
the CSQDs exhibits efficiency 2.5 times higher than neat core CdSe QDs-based device.
Finally, we managed to predict the solar cell device performance based on both electron
and hole injection dynamics. Such way to predict the device performance provides
Conclusions and future work
53
opportunity to optimize the core–shell QD materials for photovoltaics prior to making
real device.
5.2 5.2 5.2 5.2 Future workFuture workFuture workFuture work::::
In the last few years, the limiting factors in QDSCs have been more clear thanks to the
understanding of charge transfer processes. In the following paragraph we will overview
some of these factors in order to draw the possibility of future work for the QDs solar
cell applications.
First of all, based on our findings in this thesis, we revealed that establishing core–
shell structure is indispensable to diminish the hole trapping sites which are the main
restriction to the hole transfer efficiency. Therefore, study the hole dynamics, especially
the injection through the gradient shell will add more important information to
complete the full picture about charge transfer in the CSQDs system.
Secondly, better understandings for the QDs crystal structure and the way it
correlates to the electronic and the optical properties of CSQDs materials are needed.
This open the door to modify and optimize these materials not only in solar cell
applications but also in other applications such as light-emitting-diodes.
Thirdly, as for board interests in the community, engineering the CSQDs structures
to optimize the light harvesting and charge separation is needed.
Last but not least, another important building block in QDSCs: the electrolyte also
need to be noticed. Better understanding of the charge transfer and recombination
dynamics in both liquid and solid electron/hole transfer materials would be meaningful
to boost the device efficiency.
Svensk sammanfattning
54
Svensk sammanfattningSvensk sammanfattningSvensk sammanfattningSvensk sammanfattning
Balansen mellan våra energibehov och den energi som konsumeras är ej längre i
jämvikt. Därför är jakten på alternativa energikällor nödvändig. Hållbara energikällor
erbjuder ett bra alternativ till fossilbränslen. Bland många typer av hållbara energikällor
erbjuder solenergi möjligheten för mer energi än dagens konsumtion. Solceller är de
smarta verktyg som omvandlar ljusets fotoner till användbar elektricitet. Utvecklingen
av solceller har redan genomgått några generationer där två viktiga faktorer styr
marknaden. Solcellernas verkningsgrad samt produktionskostnaderna för att tillverka
dem är hörnstenar inom solcellsmarknaden. Tredje generationens solceller försöker
optimera verkningsgrad mot kostnad via billiga material som fortfarande är tillräckligt
’smarta’ för att skapa laddningsbärare när ljus absorberas och därefter genererar
elektricitet. Samtidigt som elektricitet genereras så är det också ett mål att övervinna
termodynamikens effektivitetsgräns. Nanomaterial har framkommit som byggstenar
för att samla solenergi i tredje generationens solceller. Bland dessa så har kvantprickar
visat sig vara starka kandidater eftersom de har goda egenskaper som hög
extinktionskoefficient, justerbar absorption samt möjligheten att generera och samla
flera excitoner via en enda högenergetisk foton.
Beteendet hos både fotoexciterade elektroner och dito hål bestämmer den generella
verkningsgraden hos en solcell baserad på kvantprickar. Denna avhandling presenterar
en systematisk studie av den ultrasnabba foto-aktiverade elektrondynamiken inom
kvantprickmaterial för solceller. Dessa processer inkluderar laddningsöverföring,
excitonmigration, fällnivåers laddningsbärarinfångning och deras verkan på solcellers
prestanda. De studerade materialen börjar med konventionella enkla CdSe-
kärnkvantprickar och fortsätter med Cd1−xSe1−yZnxSy-gradient-kärn–skal-kvantprickar
(CS). Det sistnämnda används för att förbättra optik- och apparatur-prestandan.
Elektroninjektionen från CdSe till ZnO-nanotrådar observerades först att hända väldigt
snabbt (några ps). Denna snabba elektroninjektionen uppmuntrar oss att studera
möjligheten att injicera multipla elektroner från en kvantprick under höga
excitationsförhållanden. Vi visade att det uppstår en konkurrens mellan
elektoninjektion och Augerrekombination.
Jämfört med elektroner så har fotoinducerade hål större sannolikhet att fångas. Men
sådana typer av fälltillstånd kan ibland vara radiativa med långa livstider, upp till några
Svensk sammanfattning
55
10-tals mikrosekunder, när de befinner sig i oleinsyratäckta CdSe-kvantprickar. I detta
scenario är hålinjektion i p-typ-kvantpricksolceller mindre effektivt (<10 %) jämfört
med elektroninjektion i motsvarande n-typ-kvantprickar. Det påverkas ytterst av fällor
på ytan som skapats av länkmolekylutbytesprocessen. Hålinjektionen kan då förbättras
genom att passivera fällorna på ytan genom att använda kärn–skalstrukturer. Utöver
elektron- eller hål-injektion kan excitonmigration också ske via FRET (Förster
resonance energy transfer, Förster-resonansenergiöverföring). Vi upptäckte att FRET
mellan kvantprickar kunde möjliggöra användning av ljusabsorption via de indirekt
kopplade kvantprickarna i QD-sensitiserade metalloxidanoder (MO). Inom
välstrukturerade blandningar av kvantprickar med olika storlekar är energiöverföring
även tydligare. Vi kunde experimentellt observera FRET-processen i slumpmässigt
arrangerade kvantprickar av olika storlekar samt i tandemstaplade QD-lager via
tidsupplösta metoder och steady state-spektroskopi. Teoretiska simuleringar där en
dipolfördelningsmodell introducerades för kopplingsberäkningar överensstämmer väl
med experimentella resultat. För att minimera effekten från defekter på ytan och
förbättra fotostabiliteten hos solceller gjorda av kvantprickar så studerade vi kärn–
skalkvantpricksystem där laddningsbärarinfångning i ytfällor kan vara väl passiverat av
skalmaterial som har förbättrade optiska egenskaper och apparaturprestanda. Här
används en halvledare med bredare bandgap som en sköld runt den aktiva kärnan i
gradienttillväxt, känt som Cd1−xSe1−yZnxSy-gradient-kärn–skal-kvantprickar. Sådana
kvantprickar erbjuder högre fotostabilitet, bättre kvantutbyte för fluorescens samt
mindre ytdefekter där materialen möts jämfört med de konventionella stegvisa kärn–
skalkvantprickarna. Först karaktäriserade vi våra CS-kvantprickar via steady state-
spektroskopi tillsammans med HR-TEM-bilder för att fastställa dimensionerna av våra
kvantprickar och utvärdera tjockleken på det skyddande skalet. Sen användes XRD och
EDX för att karaktärisera den kemiska sammansättningen samt kristallstrukturen.
Fotodynamiken hos dessa CS-kvantprickar i fotovoltaiska system studerades också.
Vi trodde först att elektroninjektionen från den aktiva kärnan till MO av n-typ visade
relativt stort exponentiellt beroende av tjockleken på skalet jämfört med stegvisa kärn–
skalkvantprickar. Vi fastställde att det högsta elektroninjektionutbytet (~80 %) kan
uppnås när skalet har en tjocklek upp till 1,3 nm. Ett sådant skal tillåter också hög
ytpassivering vilket ger optimala förhållanden för laddningsuppsamling i solceller. Till
slut integrerade vi vår kunskap om beteendet av elektroner och hål för att förklara
solcellsprestanda enligt kärn–skalstrukturer. Vi bekräftade att hålfällor är den kritiska
Svensk sammanfattning
56
faktorn för verkningsgraden hos solceller gjorda av kvantprickar. Fällornas påverkan
kan gottgöras väl genom att använda optimala kärn–skalstrukturer.
الملخص العربي
57
الملخص العربىل الشغل ثـ مي خرى للطاقة ال غنى عنه و أ أصبح البحث عن مصادر قد و ةمستمر زيادة ين استهالك العالم للطاقة فإ
بر ت عي يلذا مصادر الطاقة المتجددة أحد أهم البدائل للوقود االحفوريل مثـ ت الشاغل للعديد من الدول والحكومات. الطاقة ل مثـ ت على الطاقة. من بين العديد من مصادر الطاقة المتجددة عتمادها إ يفحجر الزاوية للعديد من الدول
من الطاقة %1فقط نأالى ا العلماء حديث توصل. لقد ةومجانيتاحة من حيث أنها م وذلك األهم المصدر الشمسية وقود.و أكهرباء إلى تحولتما ذا إالستهالك العالم كله يتكفرض األسطح ىالقـادمة إلالشمسية
ل حصد فوتونات من خال يمكنها تحويل الطاقة الشمسية الى كهرباء يالخاليا الشمسية االداة الذكية التعتبر ت . وعلى ذلك ةيكهربائالطاقة ال ة بدورها تنتقـل الى االقطاب المختلقة مولد يالتالطاقة الضوئية وتوليد حامالت للشحنة
ل للخاليا الشمسية األو ل المعادلة بين السعر والكفـاءة. قـام الجيل بهدف ح كثر من جيلأت الخاليا الشمسية بفـلقد مر في أما ،ل هذا الجيل أعلى كفـاءة حتى االن ولكن على حساب التكلفةل للضوء وسج كون كمستقب يعلى إستخدام السيل
. سجلت خاليا الجيل رلالغير متبكون يالسيلمثل ستخدام مواد رخيصة الثمن امن الخاليا الشمسية فقد تم يالجيل الثان فياءة عالية نفس الوقت لها كفـ يلة رخيصة الثمن وفدى إلى البحث عن مواد مستقب أكفـاءة ضعيفة مما يالثان
وكان هذا هو هدف الجيل الثالث من الخاليا الشمسية. ،امتصاص الطاقة الضوئية
الموصالت أشباهبرزها أالجيل الثالث من الخاليا الشمسية من فيت م خد ست إ يهناك العديد من المواد التس تجعلها مناف ةز الكوانتم دوت بخواص مميز ). تتمي نانومتر 10-8بقطر يتراوح من النانومترية (الكوانتم دوت
ر يتغي فيسهل م الحك الت –للضوء جدا يعالمتصاص إالخصائص: معامل هذمجال الخاليا الشمسية. من أهم ه في يقو من حامل كثر أيد القدرة على تول – يالطيف ياصها للضوء على المنحنمنطقة امتص فيحجمها مما يترتب عليه التحكم
عد من اإللكترون و الفجوة ب فجوة) من فوتون واحد ذو طاقة عالية. يعد مسار كال -للشحنة (زوج من إلكترونر أحد ب عت الشحنات ي هدراسة مسار هذفـإن وعليه ،حديد كفـاءة الخلية الشمسيةت يفالفوتون العبا هاما جدا متصاص ا
المواد. ههذأهم الطرق لتحسين كفـاءة الخاليا الشمسية القـائمة على
ههذتحسين خواص رضغ الفوتون ل متصاص ا ب ق من اإللكترون والفجوة ع االطروحة تم دراسة حركية كال ههذ يفنتقـال إن أالمواد. لقد تم التوصل إلى ههذالمواد قدر المستطاع لتحسين كفـاءة الخاليا الشمسية القـائمة على
بضع من ي ف يتم ةالحال ههذ يف) ZnO Nanowiresاإللكترون من الكوانتم دوت إلى مستقبل اإللكترونات (ظل استخدام فوتونات يف ة فـائقة السرعة فتحت الباب لدراسة إمكانية انتقـال إلكترون ثان يالعمل ه. هذالبيكوثانية
الملخص العربي
58
ما يعرف بإتحاد و ياإللكترون الثاننتقـال االدراسة على أن هناك منافسة بين ههذذات طاقة عالية جدا. أسفرت ).Auger Recombinationأوجر (
كفـاءة الخلية يفمن اإللكترون والفجوة بعد تفعليهما مع الضوء يلعب دورا هاما كما ذكرنا آنفـا أن مسار كال وقيفها من خالل الفجوات إذا ما تم ت ههذعمر راسة مسار الفجوة بعد االثارة. مبدئيا تم دراسة الشمسية لذلك قمنا بد
ههذ يتلك العيوب كمصائد للشحنات ولقد وجدنا أن عمر الفجوات فتعمل عيوب على سطح الكوانتم دوت. ب بعد دراسة ديناميكية إصطياد الفجوات بمصائد السطح (عيو المصائد طويل جدا (العشرات من الميكروثانية).
). توصلنا إلى أن NiOالسطح) قمنا بدراسة دينامكية إنتقـال الفجوات من الكوانتم دوت إلى مستقبل الفجوات (بتقـليل د أثبتنا أنهنتقـالها إلى المستقبل. ولقإمصائد السطح وعملية يفعملية إصطياد الفجوات بين يهناك تنافس قو
المصائد على سطح الكوانتم دوت تزداد عملية انتقـال الفجوات من الكوانتم دوت إلى المستقبل من هعدد هذ. من الطرق المعروفة لتقـليل عدد المصائد على سطح الكوانتم دوت استخدام غطاء من شبة موصل %50إلى 10%
).Core–shell quantum dots) أوسع (band gapذو (
نفصال وهوإلالفجوة قبيل ا –وهو عبارة عن زوج من اإللكترون excitonاألطروحة بعد ذلك حركية التناقش ال الطاقة وجود مستقبل لإللكترونات حيث يتم إنتقـ يالدراسة ف هنتقـال الطاقة أو هجرة الطاقة. تمت هذاعرف بما ي
خيرا إلى تم فصل الشحنات وتنتقـل اإللكترونات أ م إلى جارتها كبيرة الحجم ومن ثم يمن الكوانتم دوت صغيرة الحج. )Size distributionإلى طريقة التحضير ( يعودجدير بالذكر أن اختالف حجم الكوانتم دوت من الالمستقبل.
ام مختلفة من الكوانتم د ألحجتعم مستقبل لإللكترونات وبعمل رص م غياب يفتم إستكمال الدراسة ولكن ثم بعد ذلك دوت.
ات لفترات هو عامل الثبتطبيقـات الخاليا الشمسية يفتحد من إستخدام الكوانتم دوت يمن أهم العوامل الت–Coreبناء غطاء من شبه موصل أخر ( المواد هو كما ذكرنا سابقـا هوأكثر الطرق كفـاءة لزيادة ثبات هذ ،طويلة
shell quantum dots.( بناء الغطاء بطريقتين عموما يتم: ) األولى يكون فيها التحول من القـلبCore إلى ( Interfacialالحد الفـاصل بين القـلب والغطاء ( يف) حاد مما يسفر عن تكوين عيوب داخلية Shellالغطاء (
defects( يدريجتبشكل تعمل كمصائد للشحنات. الثانية يكون فيها التحول من القـلب إلى الغطاء يوالت )Gradient core–shell quantum dots.ن الجزء اآلخر إوعليه فـ ) وهو ما يؤدى إلى تقـليل العيوب الداخلية
تم دراسة من األطروحة قـائم على دراسة حركية كال من اإللكترونات و الفجوات عقب امتصاص الفوتون. مبدئيا ZnO( إلى المستقبل) Gradient core–shell quantum dots(إنتقـال اإللكترون من الكوانتم دوت
Nanoparticles (هذا الغطاء تأثير سماكة ) ودراسةShell thickness ( على إنتقـال االلكترونات. تم التوصلر حماية عالية وف ت نفس الوقت يفو على كفـاءة إنتقـال اإللكترونات ي السماكة التي ال تؤثروه سماكة المثلى إلى ال
من عيوب السطح (مصائد الشحنات).
الملخص العربي
59
) إلى Gradient core–shell quantum dotsبدراسة إنتقـال الفجوات من الكوانتم دوت (قمنا ايضا فجوات ال النتقـال ا. تم التوصل إلى أن الغطاء على إنتقـال الفجوات سماكة) ودراسة تأثير NiOمستقبل الفجوات (
شمسية. تم التوصل اليا خالالالغطاء على كفـاءة سماكةالغطاء. أخيرا قمنا بدراسة تأثير سماكةيعتمد بصورة كبيرة على يفغطاء). يأعلى من القـلب بدون أ ةمر 2.5تم تسجيل أعلى كفـاءة (نانومتر 1.3حوالى سماكةإلى أنه عند
ات.من اإللكترونات والفجو من خالل دراسة حركية كال سماكةنفس السياق تم حساب الكفـاءة المتوقعة لكل
References
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