The Astrophysical Scales Set by the Cosmological Constant, Black-Hole Thermodynamics and Non-Linear Massive Gravity

被引：20

作者：

Arraut, Ivan ^{[1
,2
,3
]}

机构：

[1] Tokyo Univ Sci, Dept Phys, Fac Sci, Shinjuku Ku, 1-3 Kagurazaka, Tokyo 1628601, Japan

[2] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan

[3] KEK Tsukuba, Ctr Theory, Inst Particle & Nucl Studies, Ibaraki 3050801, Japan

来源：

UNIVERSE | 2017年 / 3卷 / 02期

关键词：

cosmological constant; Black-hole temperature; static observers; graviton mass; Stuckelberg function; BACKGROUNDS; CREATION; MODEL; KERR;

D O I：

10.3390/universe3020045

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We calculate explicitly the black-hole temperature for the Schwarzschild de-Sitter solution inside massive gravity by defining the Killing-vector in the direction of the Stuckelberg function. We then consider the conditions which an observer in massive gravity has to obey in order to agree with the standard results of General Relativity.

引用

页数：20

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