Radiative properties for warm and hot dense matter

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 ap...

Full description

Saved in:
Bibliographic Details
Published inHigh energy density physics Vol. 7; no. 3; pp. 163 - 168
Main Authors de la Varga, A.G., Velarde, P., Cotelo, M., de Gaufridy, F., Zeitoun, P.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.09.2011
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary: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.
ISSN:1574-1818
1878-0563
DOI:10.1016/j.hedp.2011.04.008