Dirac R-matrix calculations of electron-impact excitation of neon-like krypton
We have employed the Dirac R-matrix method to determine electron-impact excitation cross sections and effective collision strengths in Ne-like Kr 26+. Both the configuration-interaction expansion of the target and the close-coupling expansion employed in the scattering calculation included 139 level...
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2008
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001 | PAPER-22277 | ||
003 | AR-BaUEN | ||
005 | 20230518205349.0 | ||
008 | 190411s2008 xx ||||fo|||| 00| 0 eng|d | ||
024 | 7 | |2 scopus |a 2-s2.0-58149306145 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
030 | |a JPAPE | ||
100 | 1 | |a Griffin, D.C. | |
245 | 1 | 0 | |a Dirac R-matrix calculations of electron-impact excitation of neon-like krypton |
260 | |c 2008 | ||
270 | 1 | 0 | |m Griffin, D. C.; Department of Physics, Rollins College, Winter Park, FL 32789, United States |
506 | |2 openaire |e Política editorial | ||
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504 | |a Berengut, J.C., Flambaum, V.V., Kozlov, M.G., (2005) Phys. Rev., 72 (4), p. 044501 | ||
504 | |a Berengut, J.C., Flambaum, V.V., Kozlov, M.G., (2006) Phys. Rev., 73 (1), p. 012504 | ||
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520 | 3 | |a We have employed the Dirac R-matrix method to determine electron-impact excitation cross sections and effective collision strengths in Ne-like Kr 26+. Both the configuration-interaction expansion of the target and the close-coupling expansion employed in the scattering calculation included 139 levels up through n = 5. Many of the cross sections are found to exhibit very strong resonances, yet the effects of radiation damping on the resonance contributions are relatively small. Using these collisional data along with multi-configuration Dirac-Fock radiative rates, we have performed collisional-radiative modeling calculations to determine line-intensity ratios for various radiative transitions that have been employed for diagnostics of other Ne-like ions. © 2008 IOP Publishing Ltd. |l eng | |
593 | |a Department of Physics, Rollins College, Winter Park, FL 32789, United States | ||
593 | |a Instituto de Astronomía y Física Del Espacio, Departamento de Física, Universidad de Buenos Aires, Argentina | ||
593 | |a School of Physics, University of New South Wales, Sydney 2052, Australia | ||
690 | 1 | 0 | |a ELECTRIC EXCITATION |
690 | 1 | 0 | |a ELECTRON ENERGY LEVELS |
690 | 1 | 0 | |a ELEMENTARY PARTICLES |
690 | 1 | 0 | |a IMPACT IONIZATION |
690 | 1 | 0 | |a INERT GASES |
690 | 1 | 0 | |a KRYPTON |
690 | 1 | 0 | |a RADIATION EFFECTS |
690 | 1 | 0 | |a RESONANCE |
690 | 1 | 0 | |a SOUND REPRODUCTION |
690 | 1 | 0 | |a COLLISION STRENGTHS |
690 | 1 | 0 | |a COUPLING EXPANSIONS |
690 | 1 | 0 | |a CROSS SECTIONS |
690 | 1 | 0 | |a IMPACT EXCITATIONS |
690 | 1 | 0 | |a INTENSITY RATIOS |
690 | 1 | 0 | |a INTERACTION EXPANSIONS |
690 | 1 | 0 | |a MATRIX CALCULATIONS |
690 | 1 | 0 | |a MATRIX METHODS |
690 | 1 | 0 | |a RADIATION DAMPING |
690 | 1 | 0 | |a RADIATIVE RATES |
690 | 1 | 0 | |a RADIATIVE TRANSITIONS |
690 | 1 | 0 | |a SCATTERING CALCULATIONS |
690 | 1 | 0 | |a STRONG RESONANCES |
650 | 1 | 7 | |2 spines |a NEON |
700 | 1 | |a Ballance, C.P. | |
700 | 1 | |a Mitnik, D.M. | |
700 | 1 | |a Berengut, J.C. | |
773 | 0 | |d 2008 |g v. 41 |k n. 21 |p J Phys B At Mol Opt Phys |x 09534075 |w (AR-BaUEN)CENRE-332 |t Journal of Physics B: Atomic, Molecular and Optical Physics | |
856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-58149306145&doi=10.1088%2f0953-4075%2f41%2f21%2f215201&partnerID=40&md5=cf61e8812790e608a408cf8d3c3f1e9c |y Registro en Scopus |
856 | 4 | 0 | |u https://doi.org/10.1088/0953-4075/41/21/215201 |y DOI |
856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_09534075_v41_n21_p_Griffin |y Handle |
856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09534075_v41_n21_p_Griffin |y Registro en la Biblioteca Digital |
961 | |a paper_09534075_v41_n21_p_Griffin |b paper |c PE | ||
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963 | |a VARI | ||
999 | |c 83230 |