The emission mechanism of gamma-ray bursts from supernovae

Author:

Postavaru Octavian1ORCID,Craciun Victor M.2ORCID

Affiliation:

1. Center for Research and Training in Innovative Techniques of Applied Mathematics in Engineering, University Politehnica of Bucharest, Splaiul Independentei 313, Bucharest 060042, Romania

2. Horia Hulubei National Institute of Physics and Nuclear Engineering, P. O. Box, MG-6, Magurele, Romania

Abstract

The connection between gamma ray bursts and supernovae is studied using a temperature-dependent vacuum model. A harmonically bound particle–antiparticle system is consistent with both Hawking radiation and Casimir effect, therefore, the Maxwell–Sellmeier model correlates the speed of light to temperature. According to quantum field theory, Lorentz invariance is violated only for temperatures larger than [Formula: see text][Formula: see text]K. Introducing in the temperature distribution of a 2D simulation for a type Ia supernova the speed of light temperature dependence proposed in this paper, results a speed of light distribution. A theoretical snapshot of this distribution at an arbitrary distance is consistent with photon photo finish resulted from experiments. Variable speed of light shows that supernova could be accompanied by gamma-ray bursts.

Publisher

World Scientific Pub Co Pte Ltd

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