The emission mechanism of gamma-ray bursts from supernovae

被引：0

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.

引用

页数：9

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