Lightcurves of thermonuclear supernovae as a probe of the explosion mechanism and their use in cosmology

dc.creatorBlinnikov, S.
dc.creatorSorokina, E.
dc.date2002-12-30
dc.date.accessioned2026-07-07T02:07:02Z
dc.date.available2026-07-07T02:07:02Z
dc.descriptionThermonuclear supernovae are valuable for cosmology but their physics is not yet fully understood. Modeling the development and propagation of nuclear flame is complicated by numerous instabilities. The predictions of supernova light curves still involve some simplifying assumptions, but one can use the comparison of the computed fluxes with observations to constrain the explosion mechanism. In spite of great progress in recent years, a number of issues remains unsolved both in flame physics and light curve modeling.
dc.description9 pages, 2 figures; presented at the 3rd Sakharov Conference (Moscow, June 2002) and at the 4th Workshop "New Worlds in Astroparticle Physic" (Faro, Portugal, September 2002)
dc.identifierhttps://arxiv.org/abs/astro-ph/0212567
dc.identifierhttp://arxiv.org/abs/astro-ph/0212567
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5565
dc.subjectAstrophysics
dc.titleLightcurves of thermonuclear supernovae as a probe of the explosion mechanism and their use in cosmology
dc.typetext

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