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

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

2004-10-29

arxiv.org/abs/astro-ph/0410731v1

Astronomy and Astrophysics

Astrophysics

To appear in "1604-2004: Supernovae as Cosmological Lighthouses", Padua, June 16-19 2004, eds. Turatto et al., ASP conference

Scientific paper

Many 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.

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