Time-dependent three-dimensional spectrum synthesis for Type Ia supernovae

M. Kromer, S.A. Sim

Research output: Contribution to journalArticlepeer-review

121 Citations (Scopus)

Abstract

A Monte Carlo code (artis) for modelling time-dependent three-dimensional spectral synthesis in chemically inhomogeneous models of Type Ia supernova ejecta is presented. Following the propagation of ?-ray photons, emitted by the radioactive decay of the nucleosynthesis products, energy is deposited in the supernova ejecta and the radiative transfer problem is solved self-consistently, enforcing the constraint of energy conservation in the comoving frame. Assuming a photoionization-dominated plasma, the equations of ionization equilibrium are solved together with the thermal balance equation adopting an approximate treatment of excitation. Since we implement a fully general treatment of line formation, there are no free parameters to adjust. Thus, a direct comparison between synthetic spectra and light curves, calculated from hydrodynamic explosion models, and observations is feasible. The code is applied to the well-known W7 explosion model and the results tested against other studies. Finally, the effect of asymmetric ejecta on broad-band light curves and spectra is illustrated using an elliptical toy model.
Original languageEnglish
Pages (from-to)1809-1826
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume398
Issue number4
DOIs
Publication statusPublished - 01 Oct 2009

Bibliographical note

Copyright 2009 Elsevier B.V., All rights reserved.

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