Physical equivalence between the covariant and physical graviton two-point functions in de Sitter spacetime

被引:34
|
作者
Faizal, Mir [1 ]
Higuchi, Atsushi [2 ]
机构
[1] Univ Durham, Ctr Particle Theory, Dept Math Sci, Durham DH1 3LE, England
[2] Univ York, Dept Math, York YO10 5DD, N Yorkshire, England
来源
PHYSICAL REVIEW D | 2012年 / 85卷 / 12期
关键词
FIELD-THEORY; PROPAGATOR; PERTURBATIONS; INSTABILITY;
D O I
10.1103/PhysRevD.85.124021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is known that the covariant graviton two-point function in de Sitter spacetime is infrared-divergent for some choices of gauge parameters. On the other hand, it is also known that there are no infrared divergences requiring an infrared cutoff for the physical graviton two-point function for this spacetime in the transverse-traceless-synchronous gauge in the global coordinate system. We show in this paper that the covariant graviton Wightman two-point function with two gauge parameters is equivalent to the physical one in the global coordinate system in the sense that they produce the same two-point function of any local gauge-invariant tensor linear in the graviton field such as the linearized Weyl tensor. This confirms the fact, pointed out decades ago, that the infrared divergences of the graviton two-point function in the covariant gauge for some choices of gauge parameters are a gauge artifact in the sense that they do not contribute to the Wightman two-point function of any local gauge-invariant tensor field in linearized theory.
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