Experimental data for electron-impact ionization, electron-ion ......Photoionization of W3+ ions:...
Transcript of Experimental data for electron-impact ionization, electron-ion ......Photoionization of W3+ ions:...
Experimental data for
electron-impact ionization,
electron-ion recombination and
photoionization of tungsten ions
3rd Research Coordination Meeting on
Spectroscopic and Collisional Data for W from 1 eV to 20 keV
IAEA, Vienna, October 07 – 09, 2014
Alfred Müller
Institut für Atom- und Molekülphysik
JUSTUS-LIEBIG- UNIVERSITÄT GIESSEN
I M PA
Outline
I. Introduction
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
Outline
I. Introduction atomic data needs – atomic data situation
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
Evolution of tungsten ion charge states in a plasma
T Pütterich, R Neu, R Dux, A D Whiteford, M G O’Mullane and the ASDEX Upgrade Team Plasma Phys. Control. Fusion 50 (2008) 085016
rate coefficients for ionization and recombination required Ionization: CADW calculations of Loch et al. (2005) Recombination: Burgess – Bethe (1965 – 1976) with ad hoc modifications
Tungsten spectroscopy in ITER
spectrometers
plasma
N. J. Peacock et al., Can. J. Phys. 86, 277 (2008)
Spectroscopic data for tungsten are needed
Data situation
Theoretical predictions for
ionization and recombination
of complex many-electron ions
such as Wq+ ( with q << Z )
have been unreliable in the past.
Experiments were (and still are) needed to
test and to guide theoretical approaches
electron-impact ionization of Wq+
photoionization of Wq+
electron-ion recombination of Wq+
e + Wq+ ® W(q+1)+ + 2e : q = 1,…,10
hn + W ® W+ + e : q = 0
e + Wq+ ® W(q-1)+ + hn (time-reversed photoionization)
no absolute cross section measurements available
Before this CRP: experimental cross section data
available for
Example of existing experimental data:
electron-impact ionization of W1+
10 100 1000
0
5
10
15
20
25
30
s1,2
for W1+
Stenke et al. 1995 Montague & Harrison 1984
Cro
ss s
ect
ion
(
10
-17 c
m2 )
Electron-ion collision energy ( eV )
Both experiments used crossed-beams techniques
Ioniz
atio
n t
hre
shold
of
gro
und-s
tate
W+
the presence of long-lived metastable ions is a general issue
Example of existing theoretical data:
electron-impact ionization of W5+
Experiment: M. Stenke, K. Aichele, D. Hathiramani, G. Hofmann, M. Steidl, R. Völpel, and E. Salzborn, J. Phys. B 28, 2711 (1995) Theory: M. S. Pindzola, D. C. Griffin, Phys. Rev. A 56, 1654 (1997)
CADW theory looks quite good but did not account for the metastables
The only previously existing data for photoionization
of tungsten atoms or ions
30 35 40 45 50 55 60 650
10
20
30
40
50
60absorption data
of Costello et al. normalized to MBPT theory
MBPT calculation by Boyle et al. shifted by -3 eV
Cro
ss s
ect
ion (
Mb )
Photon energy ( eV )
Experiment: J.T. Costello, E.T. Kennedy, B.F. Sonntag, C.L. Cromer, J. Phys. B 24, 5063 (1991) Theory: J. Boyle, Z. Altun and H.P. Kelly, Phys. Rev. A 7, 4811 (1993)
Outline
I. Introduction
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
Principle of electron-ion merged beams experiments
independently absolute cross sections and rate coefficients obtained
electron
beam
Ion
beam
A(q-1)+
charge-state
analyzer
long interaction path
Recombination of Wq+ ions using the TSR ring
TSR ion storage ring in Heidelberg unique facility with optimal features for the purpose cooler plus target excellent energy resolution
The storage ring TSR
The TSR has been shut down but might be moved to CERN A cryogenic electrostatic ring (CSR) is being built in Heidelberg Even a storage ring cannot guarantee the absence of metastables
Excited-state population in a beam of W18+ ions
K. Spruck, N. R. Badnell, C. Krantz, O. Novotný, A. Becker, D. Bernhardt, M. Grieser, M. Hahn, R. Repnow, D. W. Savin, A. Wolf, A. Müller, and S. Schippers, Phys. Rev. A 90, 032715 (2014)
1671 levels in configurations 4f10, 4f9 5s, 4f9 5p
sum of 1652 short-lived levels
4d10 4f10
4d10 4f10 (t »12 years)
(DR of excited levels normally suppressed by strong autoionization)
17 long-lived levels from 4f10 and 4f9 5s configurations
Metastable ions can be present even in storage-ring experiments
Recombination of W20+ ions at the TSR storage ring
S. Schippers et al., Phys. Rev. A 83, 012711 (2011)
huge recombination at low energies
26.09.2014: 31 citations in google scholar
Plasma recombination rate coefficient of W20+ ions
S. Schippers et al., Phys. Rev. A 83, 012711 (2011)
Theory for W20+
N. R. Badnell, C. P. Ballance, D. C. Griffin, M. O’Mullane, PRA 2012
fine structure included (IC)
4d®4f contribution (IC)
no fine structure (LS-coupling)
TSR
TSR
statistical approach (full mixing) see also: V. A. Dzuba, V. V. Flambaum, G. F. Gribakin, C. Harabati, PRA 2012
Recombination of W18+ ions: Just published K. Spruck, N. R. Badnell, C. Krantz, O. Novotný, A. Becker,
D. Bernhardt, M. Grieser, M. Hahn, R. Repnow, D. W. Savin, A. Wolf, A. Müller, and S. Schippers, Phys. Rev. A 90, 032715 (2014)
PD: „partitioned and damped“ ST: statistical theory (Dzuba et al. 2012) IC: intermediate coupling RR: radiative recombination
Plasma recombination rate coefficient of W18+ ions: Just published
K. Spruck, N. R. Badnell, C. Krantz, O. Novotný, A. Becker, D. Bernhardt, M. Grieser, M. Hahn, R. Repnow, D. W. Savin, A. Wolf, A. Müller, and S. Schippers, Phys. Rev. A 90, 032715 (2014)
Further DR measurements for W19+ and W21+ ions are under analysis
Experimental Cooperation Working on
Wq+ Recombination
IAMP, Giessen
Stefan Schippers Kaija Spruck Dietrich Bernhardt Alfred Müller
MPI-K, Heidelberg
M. Grieser, C. Krantz, R. Repnow, A. Wolf Columbia University, Astronomy &
Astrophysics, New York
M. Hahn, O. Novotný, D. W. Savin GSI Helmholtz Center, Darmstadt
M. Lestinsky
Arno Becker
Outline
I. Introduction
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
ion source
Overview of the experimental setup at the ALS
IAMP in collaboration with
R. A. Phaneuf et al.,
University of Nevada, Reno
Photoionization of W+ and W2+ ions: absolute data
20 40 60 80 1000
10
20
30
40
PI
cro
ss s
ect
ion
(M
b)
Photon energy (eV)
hn + W+ ® W
2+ + e
100 meV resolution
40 50 60 70 800
1
2
3
4
5
6
7
hn + W+ ® W
3+ + e
100 meV resolution
PI cr
oss
se
ctio
n (
Mb
)
Photon energy (eV)
20 30 40 50 60 70 800
20
40
60 hn + W2+
® W3+
+ e-
100 meV resolution
PI cr
oss
se
ctio
n (
Mb
)
Photon energy (eV)
60 70 800
1
2
3
4
5
PI
cro
ss s
ect
ion
(M
b)
Photon energy (eV)
hn + W2+
® W4+
+ 2e-
100 meV resolution
Photoionization of W3+ ions: experiment and theory
30 40 50 60 70 800
20
40
60
80 normalized ALS absolute ALS DARC173cc:
stat. weighted 4F states
convoluted with 100 meV gaussian shifted by -2.0 eV
PI
cro
ss s
ect
ion (
Mb
)
Photon energy (eV)
W3+
(4f14
5s25p
65d
3 4F
3/2) is g.s.
Photoionization of W3+ ions: 379-level calculation
B. M. McLaughlin and C. P. Ballance
The higher-order calculation takes care of the energy shift and some of the remaining discrepancy.
40 45 50 55 60 65 70 75 80 85 900
50
100
150
200
J=3J=4
J=2
J=3
J=2
J=1
J=2
5p
6 5
d6s
1D
2
5p
6 5
d6s
3D
J
J=4
J=3
experiment theory
Cro
ss s
ect
ion
( M
b )
Photon energy ( eV )
J=2
5p
6 5
d2 3
FJ
J=4
J=3
J=2
50 52 54 56 58 60 620
50
100
150
contributions of individual fine-structure states
W4+
500 meV resolution
Photoionization of W4+ ions:experiment and theory
Theory (52-levels close-coupling Dirac-Coulomb R-matrix calculations): C. P. Ballance and B. M. McLaughlin Calculations for Wq+ with q=0,1,2,3,4 and with up to 392 levels are underway
Experiment (200 meV and 500 meV resolution measurements available)
Photoionization of W5+: a nightmare for theory
20 30 40 50 60 70 80 90 100 1100
10
20
30
ion
iza
tion
th
resh
old
of th
e
4f1
45
d g
rou
nd
sta
te
hn + W 5+
® W 6+
+ eat 100 meV resolution
Cro
ss s
ect
ion (
Mb )
Photon energy ( eV )
ionization thresholds of the
126 levels in the excited 4f13
5d2
and 5p54f
145d
2 configurations
The huge number of possible metastable levels calls for a new different theoretical approach
Photoionization of W5+: detail of measured spectrum
71 72 73 74 75 76 770
10
20
30
hn + W 5+
® W 6+
+ eat 100 meV resolution
Cro
ss s
ect
ion
(
Mb
)
Photon energy ( eV )
It is all real resonances
Experimental Cooperation Working on
Wq+ Photoionization
IAMP, Giessen
Alfred Müller, Stefan Schippers Jonas Hellhund
Physics Department, UNR, Reno
R. A. Phaneuf Advanced Light Source, Berkeley
A. L. D. Kilcoyne
Outline
I. Introduction
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
Versatile apparatus
for studying atomic
collisions
Electron-ion crossed-
beams setup at IAMP
Electron-ion interaction region
cathode
ions
collector
energy-defining electrode
electron current: 450 mA at 1 keV
Electron-impact single ionization of W5+ ions
10 100 1000
0
1
2
3
4
5
6e + W
5+ ® W
6+ + 2e
Cro
ss s
ect
ion
(
10
-17cm
2 )
Electron-ion collision energy [eV]
Stenke et al., 1994
g.s
. th
resh
old
Electron-impact single ionization of W5+ ions
10 100 1000
0
1
2
3
4
5
6
g.s
. th
resh
old
e + W 5+
® W 6+
+ 2e
Cro
ss s
ect
ion
(
10
-17cm
2 )
Electron-ion collision energy [eV]
Stenke et al., 1994
present absolute
Electron-impact single ionization of W5+ ions
10 100 1000
0
1
2
3
4
5
6
g.s
. th
resh
old
e + W 5+
® W 6+
+ 2e
Cro
ss s
ect
ion
(
10
-17cm
2 )
Electron-ion collision energy [eV]
Stenke et al., 1994
present absolute
present scan
Electron-impact single ionization of W5+ ions
10 100 1000
0
1
2
3
4
5
6
g.s
. th
resh
old
e + W 5+
® W 6+
+ 2e
Cro
ss s
ect
ion
(
10
-17cm
2 )
Electron-ion collision energy [eV]
Stenke et al., 1994
present absolute
present scan
theory V. Jonauskas
24% metastables
Electron-impact single ionization of W8+, W11+, and
W12+ ions
200 400 600 800 1000
0
5
10
W8+
W11+
W12+
Cro
ss s
ect
ion
(
Mb
)
Electron-ion collision energy ( eV )
Electron-impact single ionization of W19+ ions
The experimental absolute cross sections can be nicely reproduced by CADW calculations
400 500 600 700 800 900 1000
0.0
0.5
1.0
1.5
2.0
2.5
e + W19+
® W20+
+ 2e
4f8
5s
I.P
.
Direct ionization: 4f, 4d, 4p
Excitation autoionization: 4d, 4p, 4s
Direct Ionization: 5s, 4f, 4d, 4pCro
ss s
ect
ion (
10
-18 c
m2 )
Electron-ion collision energy ( eV )
Excitation-autoionization: 4f, 4d, 4p, 4sGround-state
Excited 4f85s
gro
und-s
tate
I.P
.
Plasma rate coefficients for electron-impact single
ionization of W19+ ions
4 5 6 7 8 91E-5
1E-4
1E-3
0.01
0.1
Ground configuration Mix of ground- and excited
Pla
sma r
ate
coeff
icie
nt
( 10
-10 c
m3s-1
)
Electron temperature ( 105 K )
40 50 60 70 80
Electron energy ( eV )
Electron-impact
ionization of low
to moderately
charged Wq+ ions:
q = 1,2,3,…,19
10 100 1000
1
2
3
4
W3+
W13+
W15+
W5+
x 55
x 55
x 50
x 45
x 40
x 20
x 13
x 6
x 3
x 2.2
x 2.2
W+
x 60
x 1.6
x 30
x 25
W8+
W11+
W17+
W19+
Electron-ion collision energy ( eV )
s (
10
-16 c
m2 )
all scan measurements are from the present tungsten ion project; the red curves cover „the new terrain“ we can provide reliable rate coefficients for ground-state ionization on the basis of CADW modeling of the data
Group involved in the measurements on electron-
impact ionization of Wq+ ions
IAMP Giessen
Alexander Borovik Kaija Spruck Arno Becker Daniel Schury Benjamin Ebinger Joachim Rausch Stefan Schippers Kurt Huber Alfred Müller
Outline
I. Introduction
II. Electron-ion recombination of Wq+ ions
III. Photoionization of Wq+ ions
IV. Electron impact ionization of Wq+ ions
V. Summary
Summary
Completed work on Wq+ ions (absolute experimental cross sections with accompanying theoretical work and plasma rate coefficients)
recombination: W18+, W19+, W20+, W21+ photoionization:
electron impact
ionization: verified and complemented work by Stenke et al. for single ionization of Wq+, q=1,2,…,10 added new theoretical background and
W1+ s1®2 , s1®3 , s1®4
W2+ s2®3 , s2®4
W3+ s3®4
W4+ s4®5
W5+ s5®6
Summary
electron impact ionization: (cross sections and rate
coefficients - new terrain)
W11+ s11®12
W12+ s12®13 W13+ s13®14 W14+ s14®15 W15+ s15®16 W16+ s16®17 W17+ s17®18 , s17®19 W18+ s18®19 W19+ s19®20
Thank you
for your
attention!