The emission mechanism of gamma-ray bursts from supernovae

被引：1
作者：
Postavaru, Octavian [1 ]
Craciun, Victor M. [2 ]
机构：
[1] Univ Politehn Bucuresti, Ctr Res & Training Innovat Tech Appl Math Engn, Splaiul Independentei 313, Bucharest 060042, Romania
[2] Horia Hulubei Natl Inst Phys & Nucl Engn, MG-6, Magurele, Romania
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2024年 / 33卷 / 09N10期
关键词：
Vacuum model; gamma ray bursts; supernovae; ERROR BOX; MODEL;
D O I：
10.1142/S0218271824500330
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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 4x109K. 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.
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页数：9
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