Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/130502
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dc.contributor.authorGallardo-Diaz, E.en_US
dc.contributor.authorMancini, R. C.en_US
dc.contributor.authorCarpenter, K. R.en_US
dc.contributor.authorAdrian, P.en_US
dc.contributor.authorFrenje, J.en_US
dc.contributor.authorFlorido Hernández, Ricardo Jesúsen_US
dc.date.accessioned2024-05-17T15:19:24Z-
dc.date.available2024-05-17T15:19:24Z-
dc.date.issued2024en_US
dc.identifier.issn1070-664Xen_US
dc.identifier.otherWoS-
dc.identifier.urihttp://hdl.handle.net/10553/130502-
dc.description.abstractKr 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.languageengen_US
dc.relation.ispartofPhysics of Plasmasen_US
dc.sourcePhysics Of Plasmas [ISSN 1070-664X], v. 31 (3), (Marzo 2024)en_US
dc.subject22 Físicaen_US
dc.subject.otherImplosion Core Conditionsen_US
dc.subject.otherLinesen_US
dc.titleTemperature and density dependence of Kr L-shell spectrum in hot dense plasmasen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1063/5.0190238en_US
dc.identifier.isi001185891400002-
dc.identifier.eissn1089-7674-
dc.identifier.issue3-
dc.relation.volume31en_US
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.contributor.daisngid8185971-
dc.contributor.daisngid15635318-
dc.contributor.daisngid14930096-
dc.contributor.daisngid27990579-
dc.contributor.daisngid37968054-
dc.contributor.daisngid56112095-
dc.description.numberofpages9en_US
dc.utils.revisionen_US
dc.contributor.wosstandardWOS:Gallardo-Diaz, E-
dc.contributor.wosstandardWOS:Mancini, RC-
dc.contributor.wosstandardWOS:Carpenter, KR-
dc.contributor.wosstandardWOS:Adrian, P-
dc.contributor.wosstandardWOS:Frenje, J-
dc.contributor.wosstandardWOS:Florido, R-
dc.date.coverdateMarzo 2024en_US
dc.identifier.ulpgcen_US
dc.contributor.buulpgcBU-BASen_US
dc.description.sjr0,708
dc.description.jcr2,0
dc.description.sjrqQ1
dc.description.jcrqQ3
dc.description.scieSCIE
dc.description.miaricds11,0
item.fulltextCon texto completo-
item.grantfulltextopen-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.orcid0000-0001-7428-6273-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.fullNameFlorido Hernández, Ricardo Jesús-
Colección:Artículos
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