Identificador persistente para citar o vincular este elemento:
http://hdl.handle.net/10553/130502
Campo DC | Valor | idioma |
---|---|---|
dc.contributor.author | Gallardo-Diaz, E. | en_US |
dc.contributor.author | Mancini, R. C. | en_US |
dc.contributor.author | Carpenter, K. R. | en_US |
dc.contributor.author | Adrian, P. | en_US |
dc.contributor.author | Frenje, J. | en_US |
dc.contributor.author | Florido Hernández, Ricardo Jesús | en_US |
dc.date.accessioned | 2024-05-17T15:19:24Z | - |
dc.date.available | 2024-05-17T15:19:24Z | - |
dc.date.issued | 2024 | en_US |
dc.identifier.issn | 1070-664X | en_US |
dc.identifier.other | WoS | - |
dc.identifier.uri | http://hdl.handle.net/10553/130502 | - |
dc.description.abstract | Kr L-shell spectroscopy modeling results are discussed in this paper, focusing on the n = 4 to n = 2 line transitions of Be- and Li-like Kr ions. Collisional radiative atomic kinetic and Stark-broadened spectral line shape calculations show electron temperature T (e )and density n (e) sensitivity in the spectrum. The combination of the T e dependence due to the relative intensity of Be-like to Li-like line emissions in the range from 1.5 to 3 keV and the n e sensitivity from the Stark broadening effect on the line shapes in the range from 5 x 10( 23 )to 2 x 10 (24) / cc results in a spectrum that can be employed to diagnose T e and n e. Two different collisional radiative atomic kinetic models i.e., Prismspect [J. J. MacFarlane, et al., Int. Fusion Sci. Appl. Conf. Proc. 457 (2003)] and ABAKO [Florido, et al., PRE, 80, 056402 (2009)] produce similar results in level populations and spectra. In x-ray spectroscopy of implosion cores, this Kr L-shell spectrum may prove useful in an intermediate T e range in which Ar is too ionized for its K-shell to be of diagnostic value and Kr is not ionized enough for its K-shell emission to be useful. | en_US |
dc.language | eng | en_US |
dc.relation.ispartof | Physics of Plasmas | en_US |
dc.source | Physics Of Plasmas [ISSN 1070-664X], v. 31 (3), (Marzo 2024) | en_US |
dc.subject | 22 Física | en_US |
dc.subject.other | Implosion Core Conditions | en_US |
dc.subject.other | Lines | en_US |
dc.title | Temperature and density dependence of Kr L-shell spectrum in hot dense plasmas | en_US |
dc.type | info:eu-repo/semantics/Article | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1063/5.0190238 | en_US |
dc.identifier.isi | 001185891400002 | - |
dc.identifier.eissn | 1089-7674 | - |
dc.identifier.issue | 3 | - |
dc.relation.volume | 31 | en_US |
dc.investigacion | Ciencias | en_US |
dc.type2 | Artículo | en_US |
dc.contributor.daisngid | 8185971 | - |
dc.contributor.daisngid | 15635318 | - |
dc.contributor.daisngid | 14930096 | - |
dc.contributor.daisngid | 27990579 | - |
dc.contributor.daisngid | 37968054 | - |
dc.contributor.daisngid | 56112095 | - |
dc.description.numberofpages | 9 | en_US |
dc.utils.revision | Sí | en_US |
dc.contributor.wosstandard | WOS:Gallardo-Diaz, E | - |
dc.contributor.wosstandard | WOS:Mancini, RC | - |
dc.contributor.wosstandard | WOS:Carpenter, KR | - |
dc.contributor.wosstandard | WOS:Adrian, P | - |
dc.contributor.wosstandard | WOS:Frenje, J | - |
dc.contributor.wosstandard | WOS:Florido, R | - |
dc.date.coverdate | Marzo 2024 | en_US |
dc.identifier.ulpgc | Sí | en_US |
dc.contributor.buulpgc | BU-BAS | en_US |
dc.description.sjr | 0,708 | |
dc.description.jcr | 2,0 | |
dc.description.sjrq | Q1 | |
dc.description.jcrq | Q3 | |
dc.description.scie | SCIE | |
dc.description.miaricds | 11,0 | |
item.fulltext | Con texto completo | - |
item.grantfulltext | open | - |
crisitem.author.dept | GIR IUNAT: Interacción Radiación-Materia | - |
crisitem.author.dept | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.dept | Departamento de Física | - |
crisitem.author.orcid | 0000-0001-7428-6273 | - |
crisitem.author.parentorg | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.fullName | Florido Hernández, Ricardo Jesús | - |
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