Energy Conservation in the thin layer approximation: IV. The light curve for supernovae

Autor:	Zaninetti, Lorenzo
Rok vydání:	2021
Předmět:	Astrophysics - High Energy Astrophysical Phenomena Astrophysics - Astrophysics of Galaxies
Zdroj:	The International Journal of Astronomy and Astrophysics,2021, 11, 37-58
Druh dokumentu:	Working Paper
DOI:	10.4236/ijaa.2021.111003
Popis:	The light curves (LC) for Supernova (SN) can be modeled adopting the conversion of the flux of kinetic energy into radiation. This conversion requires an analytical or a numerical law of motion for the expanding radius of the SN. In the framework of conservation of energy for the thin layer approximation we present a classical trajectory based on a power law profile for the density, a relativistic trajectory based on the Navarro--Frenk--White profile for the density, and a relativistic trajectory based on a power law behaviour for the swept mass. A detailed simulation of the LC requires the evaluation of the optical depth as a function of time. We modeled the LC of SN~1993J in different astronomical bands, the LC of GRB 050814 and the LC GRB 060729 in the keV region. The time dependence of the magnetic field of equipartition is derived from the theoretical formula for the luminosity. Comment: 18 figures and 20 pages
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/2102.07386 Zobrazit plný text záznamu View this record from Arxiv