On Stefan-Boltzmann law and the Casimir effect at finite temperature in the Schwarzschild space-time

被引:1
|
作者
Santos, A. F. [1 ]
Ulhoa, S. C. [2 ,3 ]
Khanna, Faqir C. [4 ,5 ]
机构
[1] Univ Fed Mato Grosso, Inst Fis, BR-78060900 Cuiaba, Mato Grosso, Brazil
[2] Univ Brasilia, Int Ctr Phys, Inst Fis, BR-70910900 Brasilia, DF, Brazil
[3] Canadian Quantum Res Ctr, 204-3002,32 Ave, Vernon, BC V1T 2L7, Canada
[4] Univ Victoria, Dept Phys & Astron, 3800 Finnerty Rd, Victoria, BC V8P 5C2, Canada
[5] Univ Alberta, Theoret Phys Inst, Phys Dept, Edmonton, AB, Canada
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2020年 / 35卷 / 13期
关键词
Schwarzschild space-time; Casimir effect; Stefan-Boltzmann law; finite temperature; TFD formalism; LIE-GROUPS; FIELDS;
D O I
10.1142/S0217751X20500669
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
This paper deals with quantum field theory in curved space-time using the Thermo Field Dynamics. The scalar field is coupled to the Schwarzschild space-time and then thermalized. The Stefan-Boltzmann law is established at finite temperature and the entropy of the field is calculated. Then the Casimir energy and pressure are obtained at zero and finite temperature.
引用
收藏
页数:12
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