Radiative recombination rate coefficients for highly-charged tungsten ions
Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells, W 28 + , W 38 + , W 46 + , W 56 + , W 64 + , W 70 + , and W 72 + , as well as for the H-like ion W 73 + and the bare nucleus W 74 + . The temperature range 10 3 – 10 10 K...
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Published in: | Atomic data and nuclear data tables Vol. 96; no. 1; pp. 1 - 25 |
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Abstract | Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells,
W
28
+
,
W
38
+
,
W
46
+
,
W
56
+
,
W
64
+
,
W
70
+
, and
W
72
+
, as well as for the H-like ion
W
73
+
and the bare nucleus
W
74
+
. The temperature range
10
3
–
10
10
K
is considered. Calculations have been performed in the framework of the fully relativistic Dirac–Fock treatment of photoionization and radiative recombination processes taking into account all significant multipoles of the radiation field. We assess the influence of multipole effects on recombination rate coefficients as compared with the commonly used dipole approximation. For the first time, we show that the relativistic Maxwell–Boltzmann distribution of continuum electrons should be used at high temperature. This decreases the rate coefficient significantly compared to the nonrelativistic distribution. |
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AbstractList | Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells, W{sup 28+}, W{sup 38+}, W{sup 46+}, W{sup 56+}, W{sup 64+}, W{sup 70+}, and W{sup 72+}, as well as for the H-like ion W{sup 73+} and the bare nucleus W{sup 74+}. The temperature range 10{sup 3}-10{sup 10}K is considered. Calculations have been performed in the framework of the fully relativistic Dirac-Fock treatment of photoionization and radiative recombination processes taking into account all significant multipoles of the radiation field. We assess the influence of multipole effects on recombination rate coefficients as compared with the commonly used dipole approximation. For the first time, we show that the relativistic Maxwell-Boltzmann distribution of continuum electrons should be used at high temperature. This decreases the rate coefficient significantly compared to the nonrelativistic distribution. Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells, W 28 + , W 38 + , W 46 + , W 56 + , W 64 + , W 70 + , and W 72 + , as well as for the H-like ion W 73 + and the bare nucleus W 74 + . The temperature range 10 3 – 10 10 K is considered. Calculations have been performed in the framework of the fully relativistic Dirac–Fock treatment of photoionization and radiative recombination processes taking into account all significant multipoles of the radiation field. We assess the influence of multipole effects on recombination rate coefficients as compared with the commonly used dipole approximation. For the first time, we show that the relativistic Maxwell–Boltzmann distribution of continuum electrons should be used at high temperature. This decreases the rate coefficient significantly compared to the nonrelativistic distribution. |
Author | Nikulin, V.K. Trzhaskovskaya, M.B. Clark, R.E.H. |
Author_xml | – sequence: 1 givenname: M.B. surname: Trzhaskovskaya fullname: Trzhaskovskaya, M.B. email: Trzhask@MT5605.spb.edu organization: Petersburg Nuclear Physics Institute, Theoretical Physics Division, Gatchina 188300, Russia – sequence: 2 givenname: V.K. surname: Nikulin fullname: Nikulin, V.K. organization: Ioffe Physical Technical Institute, St. Petersburg 194021, Russia – sequence: 3 givenname: R.E.H. surname: Clark fullname: Clark, R.E.H. organization: Nuclear Data Section, International Atomic Energy Agency, Vienna A-1400, Austria |
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Cites_doi | 10.1088/0953-4075/34/16/302 10.1088/0029-5515/45/3/007 10.1103/PhysRevE.78.035401 10.1086/192284 10.1103/RevModPhys.40.441 10.1016/j.adt.2007.09.002 10.1103/PhysRev.165.253 10.1016/j.radphyschem.2003.12.019 10.1006/adnd.2002.0884 10.1088/0022-3700/13/5/017 10.1103/PhysRevA.27.2913 10.1086/508465 10.1134/1.1412672 10.1103/PhysRevA.49.1816 10.1006/adnd.1999.0825 10.1134/1.1621437 10.1016/0092-640X(86)90012-4 |
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Data Tables doi: 10.1006/adnd.1999.0825 contributor: fullname: Ichihara – volume: 95 start-page: 537 year: 2003 ident: 10.1016/j.adt.2009.08.004_bib14 publication-title: Opt. Spectrosc. doi: 10.1134/1.1621437 contributor: fullname: Trzhaskovskaya – volume: 34 start-page: 415 year: 1986 ident: 10.1016/j.adt.2009.08.004_bib3 publication-title: At. Data Nucl. Data Tables doi: 10.1016/0092-640X(86)90012-4 contributor: fullname: Clark – year: 1957 ident: 10.1016/j.adt.2009.08.004_bib21 contributor: fullname: Bethe |
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Snippet | Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells,
W
28
+
,
W
38
+
,
W
46
+
,
W... Partial and total radiative recombination rate coefficients are presented for highly-charged ions of tungsten with closed shells, W{sup 28+}, W{sup 38+}, W{sup... |
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SubjectTerms | APPROXIMATIONS ATOMIC AND MOLECULAR PHYSICS BOLTZMANN STATISTICS DIPOLES ELECTRONS MULTICHARGED IONS PHOTOIONIZATION RECOMBINATION RELATIVISTIC RANGE TUNGSTEN TUNGSTEN IONS |
Title | Radiative recombination rate coefficients for highly-charged tungsten ions |
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