On the temperature of gravitation in the de Sitter space-time

被引:1
作者
Santos, A. F. [1 ]
Ulhoa, S. C. [2 ,3 ]
Furtado, T. F. [4 ]
Khanna, Faqir C. [5 ,6 ]
机构
[1] Univ Fed Mato Grosso, Inst Fis, BR-78060900 Cuiaba, Mato Grosso, Brazil
[2] Univ Brasilia, Inst Fis, Int Ctr Phys, BR-70910900 Brasilia, DF, Brazil
[3] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada
[4] Univ Brasilia, Inst Fis, BR-70910900 Brasilia, DF, Brazil
[5] Univ Victoria, Dept Phys & Astron, 3800 Finnerty Rd, Victoria, BC, Canada
[6] Univ Alberta, Theoret Phys Inst, Phys Dept, Edmonton, AB, Canada
来源
EUROPEAN PHYSICAL JOURNAL C | 2021年 / 81卷 / 05期
关键词
D O I
10.1140/epjc/s10052-021-09189-3
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The temperature associated with gravitation as presented in the Unruh effect and Hawking temperature serves to link different areas of physics, such as gravity, statistical mechanics, and quantum physics. In this paper, teleparallel gravity is considered to study temperature effects on the de Sitter space-time. The effects of temperature are introduced using the thermo field dynamics formalism. The gravitational Stefan-Boltzmann law is obtained. Then the temperature of gravitation in the de Sitter space-time is calculated. Here an Unruh-type effect is discussed. This effect relates the temperature and the acceleration of a particle in the de Sitter space-time. The gravitational Casimir effect is calculated. The result shows that there is a transition between an attractive and a repulsive Casimir effect.
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页数:8
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