Radiative properties for warm and hot dense matter
Data(s) |
01/09/2011
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Resumo |
We will present calculations of opacities for matter under LTE conditions. Opacities are needed in radiation transport codes to study processes like Inertial Confinement Fusion and plasma amplifiers in X-ray secondary sources. For the calculations we use the code BiGBART, with either a hydrogenic approximation with j-splitting or self-consistent data generated with the atomic physics code FAC. We calculate the atomic structure, oscillator strengths, radiative transition energies, including UTA computations, and photoionization cross-sections. A DCA model determines the configurations considered in the computation of the opacities. The opacities obtained with these two models are compared with experimental measurements. |
Formato |
application/pdf |
Identificador | |
Idioma(s) |
eng |
Publicador |
E.T.S.I. Industriales (UPM) |
Relação |
http://oa.upm.es/11161/2/INVE_MEM_2011_102046.pdf http://dx.doi.org/10.1016/j.hedp.2011.04.008 info:eu-repo/grantAgreement/EC/FP7/211737 info:eu-repo/semantics/altIdentifier/doi/10.1016/j.hedp.2011.04.008 |
Direitos |
http://creativecommons.org/licenses/by-nc-nd/3.0/es/ info:eu-repo/semantics/openAccess |
Fonte |
High Energy Density Physics, ISSN 1574-1818, 2011-09, Vol. 7, No. 3 |
Palavras-Chave | #Energía Nuclear #Física |
Tipo |
info:eu-repo/semantics/article Artículo PeerReviewed |