Consistent Radiative Transfer Models including Time Dependent Energy Deposition for Type Ia Supernovae

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dc.creatorHultzsch, P.
dc.creatorSauer, D.
dc.creatorPauldrach, A. W. A.
dc.creatorHoffmann, T.
dc.date2004-10-29
dc.date.accessioned2026-07-07T02:15:35Z
dc.date.available2026-07-07T02:15:35Z
dc.descriptionMany aspects of the explosion mechanism of Type Ia supernovae (SN Ia) still remain unclear -- causing uncertainties in the derived cosmological parameters. Realistic models of the generation and transport of radiation in the ejecta are required which link theoretical explosion models to observations. We aim to construct theoretical spectra and light curves from consistent radiative transfer models that allow to study the dependence of observable features on the physical parameters of the explosion.
dc.descriptionTo appear in "1604-2004: Supernovae as Cosmological Lighthouses", Padua, June 16-19 2004, eds. Turatto et al., ASP conference Series. 2 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0410731
dc.identifierhttp://arxiv.org/abs/astro-ph/0410731
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8460
dc.subjectAstrophysics
dc.titleConsistent Radiative Transfer Models including Time Dependent Energy Deposition for Type Ia Supernovae
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