Quantum fields in the static de Sitter universe

被引:14
|
作者
Akhmedov, E. T. [1 ,2 ]
Bazarov, K., V [1 ,2 ]
Diakonov, D., V [1 ,2 ]
Moschella, U. [3 ,4 ]
机构
[1] Moscow Inst Phys & Technol, Inst Skii 9, Dolgoprudnyi 141700, Russia
[2] Inst Theoret & Expt Phys, B Cheremushkinskaya 25, Moscow 117218, Russia
[3] Univ Insubria, Dipartimento DiSAT, Via Valleggio 11, I-22100 Como, Italy
[4] Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20146 Milan, Italy
来源
PHYSICAL REVIEW D | 2020年 / 102卷 / 08期
关键词
VACUUM STATES; SCALAR FIELD; SPACE; DESITTER;
D O I
10.1103/PhysRevD.102.085003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct explicit mode expansions of various tree-level propagators in the Rindler-de Sitter universe, also known as the static (or compact) patch of the de Sitter spacetime. We construct in particular the Wightman functions for thermal states having a generic temperature T. We give a fresh simple proof that the only thermal Wightman propagator that respects the de Sitter isometry is the restriction to the Rindler-de Sitter wedge of the propagator for the Bunch-Davies state. It is the thermal state with T = (2 pi)(-1) in the units of de Sitter curvature. We show that propagators with T not equal (2 pi)(-1) are only time translation invariant and have extra singularities on the boundary of the static patch. We also construct the expansions for the so-called alpha-vacua in the static patch and discuss the flat limit.
引用
收藏
页数:14
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