2016MNRAS.459.2777R

Query : 2016MNRAS.459.2777R

2016MNRAS.459.2777R - Mon. Not. R. Astron. Soc., 459, 2777-2786 (2016/July-1)

Modelling long GRBs using a single shock with relativistic radiation hydrodynamics.

RIVERA-PALEO F.J. and GUZMAN F.S.

Abstract (from CDS):

We explore the possibility that a single relativistic shock, where the gas dynamics is coupled with radiation, can fit the light curves of long GRBs. For this, we numerically solve the 1D relativistic radiation hydrodynamics equations with a single initial shock. We calculate light curves due to the evolution of this shock in terms of the velocity of the shock, the opacity of the gas, mass density and density of radiated energy. We explore how the variation of each of these parameters provides different features in the light curves. As examples, we include the fitting of two long GRBs.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): opacity - radiative transfer - methods: numerical - gamma-ray burst: general - gamma-ray burst: general

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 060904B gB 03 52 50.520 -00 43 30.61 18.27 19.14 18.37     ~ 208 0
2 GRB 080413B gB 21 44 34.62 -19 58 51.2           ~ 191 0

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