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8/18/2019 CH30!1!6 Quantum Physics HANIM MJ
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Copyright © 2010 Pearson Education, Inc.
Chapter 30
Quantum Physics
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Copyright © 2010 Pearson Education, Inc.
Units of Chapter 30
•
Blackbody Radiation and Planck’sHypothesis of Quantized ner!y
• Photons and the Photoelectric ffect
• "he #ass and #omentum of aPhoton
• Photon $catterin! and the Compton
ffect
• "he de Bro!lie Hypothesis and
%a&e'Particle (uality
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Copyright © 2010 Pearson Education, Inc.
)t the end of the lesson* the students
should be able to+
)ckno,led!e Planck’s hypothesis that
radiation emitted and absorbed by the ,all of
a black body ca&ity is -uantized.
)ppreciate instein’s contribution to
-uantum theory and its relation to black body
radiation.
(escribe Photoelectric ffect* apply e-uationin&ol&in! ener!y of a photon* ,ork function
and ma/imum kinetic ener!y of an eected
electron.
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$tate the rest mass of a photon and its
momentum.
/plain Compton ffect -ualitati&ely.
(escribe the de Bro!lie hypothesis.
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Copyright © 2010 Pearson Education, Inc.
30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
)n ideal blackbody absorbs all the li!ht that is
incident upon it.
#ultiple
reflections causeabsorption
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Copyright © 2010 Pearson Education, Inc.
30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
/perimentally* if ,emeasure the intensity of
the electroma!netic
radiation emitted by an
ideal blackbody* ,e find+
•
"he temperature is increased2
• "he peak in the radiation shifts
to,ard hi!her fre-uency.
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↑
")rea under !raph
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30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
"his illustrates a remarkable e/perimental
findin!+
"he distribution of ener!y in blackbody
radiation is independent of the material from
,hich the blackbody is constructed itdepends only on the temperature* T .
"he peak fre-uency is !i&en by+
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30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
"he peak ,a&elen!th increases linearly ,iththe temperature 4color5.
Classical physics calculations ,erecompletely unable to produce this
temperature dependence* leadin! to
somethin! called the 6ultra&iolet
catastrophe.7
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30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
Classical predictions ,ere that the intensity
increased rapidly ,ith fre-uency* hence the
ultra&iolet catastrophe.
• (i&er!e to at hi!her f .•
BB radiates ,ith of • 8U9 catastrophe.
• Planck assume ener!y
is -uantized• (eri&e a cur&e in
a!reement ,ith
e/perimental results.
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30'1 Blackbody Radiation and Planck’s
Hypothesis of Quantized ner!y
Planck disco&ered that he could reproduce the
e/perimental cur&e by assumin! that the
radiation in a blackbody came in -uantized
ener!y packets* dependin! on the fre-uency+
"he constant h in this e-uation is kno,n as
Planck’s constant+
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30': Photons and the Photoelectric ffect
Planck relates ener!y -uantization in BB is due
to -uantized &ibration of atom in the ,all.
He did not think the -uantized ener!y come
from the li!ht itself.
instein su!!ested that the -uantization of
li!ht ,as real2 that li!ht came in small packets
or bundle of ener!y* called photons ,ith
ener!y of+
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30': Photons and the Photoelectric ffect
instein’s photon model+
#ore intense beam of li!ht ,ill contain morephotons
the ener!y of each photon does not chan!e.
Beam of light or particles of photons, each carry energy hf.
If f is constant, increasing I , result:
photons tightly packed.
At a given time, >photons pass a point, >photons shines on surface, &
↑
to the surface.
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30': Photons and the Photoelectric ffect
"he photoelectric effect occurs ,hen a beam
of li!ht strikes a metal* and electrons areeected.
ach metal has a minimum amount of ener!y
re-uired to eect an electron* called the ,ork
function* W 0.
;f the electron is !i&en an ener!y E by the
beam of li!ht* its ma/imum kinetic ener!y is+
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1e9 < 1.=/10'1>?
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30': Photons and the Photoelectric ffect
"his dia!ram sho,s the basic layout of a
photoelectric effect e/periment.
Result+ electric current
#etal plate
ectin! electrons
@i!ht shines
)ttracted to a A&e
char!ed collector plate
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30': Photons and the Photoelectric ffectClassical predictions+
1. )ny beam of li!ht of any color can eect
electrons if it is intense enou!h.
:. "he ma/imum kinetic ener!y of an eected
electron should increase as the intensity
increases.
bser&ations+
3. @i!ht must ha&e a certain minimum fre-uency*
cutoff fre-uency* f 0 in order to eect electrons.
. #ore intensity only results in more electrons of
the same ener!y 4E independent of intensity but
depend on frequency 5.
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30': Photons and the Photoelectric ffect
/planations+
1. ach photon’s ener!y is determined by itsfre-uency. ;f it is less than the ,ork function*
W o * electrons ,ill not be eected* no matter
ho, intense the beam.*minimum condition: E=W o
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30': Photons and the Photoelectric ffect
:. ) more intense beam means more photons*
and therefore more eected electrons.
• $odium and !old ha&e different cutoff fre-uencies 4due to different material5.• $lope of the t,o lines is the same2 h
30 2 Ph d h
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30-2 Photons and the
Photoelectric Efect
30 2 Ph d h
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30-2 Photons and the
Photoelectric Efect
30 3 "h # d # t f Ph t
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30'3 "he #ass and #omentum of a Photon
"he total ener!y can be ,ritten+
$ince the left side of the e-uation must be
zero for a photon* it follo,s that the ri!ht side
must be zero as ,ell.
Photons al,ays tra&el at the speed of li!ht* &
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30'3 "he #ass and #omentum of a Photon
Dinally* ,e can ,rite the momentum of a
photon in the follo,in! ,ay+
30 Ph t $ tt i d th C t
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Copyright © 2010 Pearson Education, Inc.
30' Photon $catterin! and the Compton
ffect
"he Compton effect occurs ,hen a photon
scatters off an atomic electron.
• E'ray photon scatter from an
electron 4at rest5.
• Result+ chan!e of ,a&elen!th
for the scattered photon.
• 8Compton effect.
30 Ph t $ tt i d th C t
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Copyright © 2010 Pearson Education, Inc.
30' Photon $catterin! and the Compton
ffect
;n order for ener!y to be conser&ed* the ener!yof the scattered photon plus the ener!y of the
electron must e-ual the ener!y of the incomin!
photon.
"his means the ,a&elen!th of the out!oin!
photon is lon!er than the ,a&elen!th of the
incomin! one+
30 F "h d B li H th i d %
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Copyright © 2010 Pearson Education, Inc.
30'F "he de Bro!lie Hypothesis and %a&e'
Particle (uality
;n 1>:3* de Bro!lie proposed that* as ,a&es cane/hibit particle'like beha&ior * particles should
e/hibit ,a&e'like beha&ior as ,ell 4,a&e'particle
duality5.
He proposed that the same relationship bet,een,a&elen!th and momentum should apply to
massi&e particles as ,ell as photons+
30 F "h d B li H th i d %
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Copyright © 2010 Pearson Education, Inc.
30'F "he de Bro!lie Hypothesis and %a&e'
Particle (uality
;ndeed* ,e can e&en
perform Goun!’s t,o'
slit e/periment ,ith
particles of theappropriate
,a&elen!th and find
the same diffraction
pattern.
30 F "h d B li H th i d %
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Copyright © 2010 Pearson Education, Inc.
30'F "he de Bro!lie Hypothesis and %a&e'
Particle (uality
"hese ima!es sho, the !radual creation of anelectron diffraction pattern.
lectrons arri&e at
the screen at
random locations
;ncreasin! the
number of electrons
Resultin!
interference
pattern becomes
more e&idence.
$ f Ch t 30
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$ummary of Chapter 30
• )n ideal blackbody absorbs all li!ht incident
on it. "he distribution of ener!y ,ithin it as a
function of fre-uency depends only on its
temperature.
• Dre-uency of ma/imum radiation+
• Planck’s hypothesis+
$ummary of Chapter 30
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Copyright © 2010 Pearson Education, Inc.
$ummary of Chapter 30
• @i!ht is composed of photons* each ,ith
ener!y+
• ;n terms of ,a&elen!th+
• Photoelectric effect+ photons eectelectrons from metal surface.
• #inimum ener!y+ ,ork function* W 0
• #inimum fre-uency+
$ummary of Chapter 30
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Copyright © 2010 Pearson Education, Inc.
$ummary of Chapter 30
• Photons ha&e zero rest mass.
• Photon momentum* fre-uency* and,a&elen!th+
• Compton effect+ a photon scatters off an
atomic electron* and e/its ,ith a lon!er
,a&elen!th+
$ummary of Chapter 30
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$ummary of Chapter 30
• de Bro!lie hypothesis+ particles ha&e
,a&elen!ths* dependin! on their momentum+
• @i!ht and matter display both ,a&elike
and particle'like properties.