1 Relativistic calculation of emission spectra of highly charged W ions and electron impact...
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- Slide 1
- 1 Relativistic calculation of emission spectra of highly
charged W ions and electron impact ionization cross sections of W
2006. 11. 14. Yongjoo Rhee ( ) Laboratory for Quantum Optics Korea
Atomic Energy Research Institute presentation at ADAS
yjrhee@kaeri.re.kr http://amods.kaeri.re.kr
- Slide 2
- 2 1.Electron impact ionization cross sections - W/W + -
Ionization of W and W+ by electron impact. Duck-Hee Kwon, Yong-Joo
Rhee, Yong-Ki Kim, International Journal of Mass Spectrometry, 252
pp213-221 (2006.4) 2.Emission spectra of highly charged W ions - W
33+, W 34+, W 35+, W 36+ 3. AMODS database -
http://amods.kaeri.re.kr
- Slide 3
- 3 Atomic Processes in a Fusion Plasma impurity photon plasma
particle 2 nd electron, ion, excited atom electron Mo, W, V Plasma
p, e, Be, Li, C, Ni, etc Plasma (keV) generation of elctron energy
loss of plasma plasma-wall interaction secondary electron electron
collision with plasma photon emission decrease of plasma
temperature secondary electron Diagnostic high Z (Ar, Xe, etc)
- Slide 4
- 4 (direct ionization) BEB (Binary Encounter Bethe) model N :
Orbital Occupation NumberB : Orbital Binding Energy U : Orbital
Kinetic Energy R : Rydberg Energy T : Incident Electron Energy t =
T/B u = U/B a 0 : Bohr Radius Bethe Mott Bound state Continuum
Electron Ionization energy interference (excitation-autoionization)
Electron Bound state 1 Excited state : autoionization or
photoemission First ionization limit Continuum Bound state 2 E:
excitation energy B: bound energy PWB: plane wave Born
Approximation for neutral atom CB: Coulomb Born approximation for
singly charged ion Electron Impact Ionization Cross Sections N,B,U
relativistic MCDF calculation
- Slide 5
- 5 MCDF Calculation Dirac-Fock Equation
http://amods.kaeri.re.kr/mcdf/MCDF.html PC version (2005)
Workstation version (2000) Exchange term Screened Coulomb charge
term Lagrange multipliers Multi Configuration Dirac-Fock (MCDF)
code : Jean-Paul Desclaux (Grenoble, France) Paul Indelicato
(University of Paris, France) Yong-Ki Kim (NIST, USA) -
ralativistic wave functions - electric and magnetic multipole
transition - plane wave Born cross section - angular coefficients,
etc Radial function X r
- Slide 6
- 6 Atom Configuratio n LS termLevel(eV) Ionization energy (eV) W
5d 4 6s 25 D 0 (g)0 7.864 5d 5 6s 7 S 3 (m)0.3659 5d 4 6s 23 P 1
(m)1.6499 W+W+ 5d 4 6s 6 D 1/2 (g)016.35 5d 5 6 S 5/2 (m)0.9200 5d
3 6s 24 F 5/2 (m)1.0801 Energy levels of W (Z=74, m=meta stable
state, g=ground state)
- Slide 7
- 7 e-impact ionization of W + ion
- Slide 8
- 8 e-impact ionization of neutral W
- Slide 9
- 9 Online calcuation of Direct Ionization Cross Section
- Slide 10
- 10 C. Biedermann, Physica Scripta, 2001 4p 6 4d n [4p 5 4d n+1
+ 4p 6 4d n-1 4f] Series of EUV spectra of W ions (25+ to 36+)
measured at Berlin EBIT Calculation by HULLAC code Emission spectra
of Highly Charged W Ions
- Slide 11
- 11 Energy levels of highly charged W ions W 36+ Mo V W 35+ Mo
IV W 34+ Mo III W 33+ Mo II
- Slide 12
- 12 Transition Probabilities of W 33+ Electric Dipole transition
only 4p 6 4d n [ 4p 5 4d n+1 + 4p 6 4d n-1 4f ] n=2 for W 36+ J= 2,
3, 4 n=3 for W 35+ J= 1/2, 3/2, 5/2 n=4 for W 34+ J= 0, 1, 2 n=5
for W 33+ J= 1/2, 3/2, 5/2
- Slide 13
- 13 Spectrum of highly charged W 33+ ions Electric Dipole
transition only 4p 6 4d n [ 4p 5 4d 6 + 4p 6 4d 4 4f ]
- Slide 14
- 14 Transition Probabilities of W 34+ Electric Dipole transition
only 4p 6 4d n [ 4p 5 4d n+1 + 4p 6 4d n-1 4f ] n=2 for W 36+ J= 2,
3, 4 n=3 for W 35+ J= 1/2, 3/2, 5/2 n=4 for W 34+ J= 0, 1, 2 n=5
for W 33+ J= 1/2, 3/2, 5/2
- Slide 15
- 15 Spectrum of highly charged W 34+ ions Electric Dipole
transition only 4p 6 4d n [ 4p 5 4d 5 + 4p 6 4d 3 4f ]
- Slide 16
- 16 Transition Probabilities of W 35+ Electric Dipole transition
only 4p 6 4d n [ 4p 5 4d n+1 + 4p 6 4d n-1 4f ] n=2 for W 36+ J= 2,
3, 4 n=3 for W 35+ J= 1/2, 3/2, 5/2 n=4 for W 34+ J= 0, 1, 2 n=5
for W 33+ J= 1/2, 3/2, 5/2
- Slide 17
- 17 Spectrum of highly charged W 35+ ions Electric Dipole
transition only 4p 6 4d n [ 4p 5 4d 4 + 4p 6 4d 2 4f ]
- Slide 18
- 18 W 33+ W 34+ W 35+ W 36+ Spectra of highly charged W ions
Electric Dipole transition only 4p 6 4d n [ 4p 5 4d n+1 + 4p 6 4d
n-1 4f ] n=2 for W 36+ J= 2, 3, 4 n=3 for W 35+ J= 1/2, 3/2, 5/2
n=4 for W 34+ J= 0, 1, 2 n=5 for W 33+ J= 1/2, 3/2, 5/2 HCI Spectra
are calculated using MCDF code for gA of each transition line and
convolution with =0.138 is performed.
- Slide 19
- 19 Spectra of highly charged W ions ASDEX upgrade, R. Neu,
J.Phys.B, At. Mol. Opt. Phys. 1997
- Slide 20
- 20 Spectra of highly charged W ions RELAC code, R. Neu,
J.Phys.B, At. Mol. Opt. Phys. 1997
- Slide 21
- 21 AMODS database http://amods.kaeri.re.kr
- Slide 22
- 22 Structure & Raw Data Sources of AMODS AMODS Atomic
Structure & TransitionsCollisions and Reactions ASL TP AEL ATL
MCDF ON-LINE POP DYNAMICS Mirror NIST ASD ALLADIN e IMPACT ISOTOPE
DATA MPI PATH NIFS AI IAEA,ORNL Michigan NIST, CUP NIFS CDS NIST
KAERI NIST ADAS KAERI Strathclyde Most data retrievals are
controlled by SCRIPTS (PERL, k-shell) Fundamental Const NIST IFE
Simulation KAERI
- Slide 23
- 23 Atomic Spectral Lines - I
- Slide 24
- 24 Atomic Spectral Lines - II
- Slide 25
- 25 Electron Impact Excitation/Ionization
- Slide 26
- 26 Electron Impact Differential Cross Section Implemented in
NIFS under CUP
- Slide 27
- 27 KAERI NIFS collaboration
- Slide 28
- 28 Dielectronic Satellite Lines - NIFS
- Slide 29
- 29 Mirror Site of NIST ASD
- Slide 30
- 30 SUMMARY Usage of W is expanding - ITER, ASDEX, TRIAM, etc -
DATA of W are necessary electron impact ionization cross section
spectra of highly charged ions MCDF code is a good tool to solve
the problem - Relativistic calculation - ab initio calculation
Verification of Data by experiments and theory is necessary - by
MCDF - in LHD,TRIAM,ASDEX-U - in laser facilities International
collaboration Japan (NIFS, ILE) China (LFRC, SIOM) Europe (ASDEX-U,
JET)