Black holes in Lorentz-violating gravity theories

被引:76
作者
Barausse, Enrico [1 ]
Sotiriou, Thomas P. [2 ,3 ]
机构
[1] Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France
[2] SISSA, I-34136 Trieste, Italy
[3] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy
基金
欧洲研究理事会;
关键词
ROTATING RELATIVISTIC STARS; GRAVITATIONAL COLLAPSE; MAXIMUM MASS; EVOLUTION; SPIN; CONSTRAINTS; ACCRETION; ETHER;
D O I
10.1088/0264-9381/30/24/244010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Lorentz symmetry and the notion of light cones play a central role in the definition of horizons and the existence of black holes. Current observations provide strong indications that astrophysical black holes do exist in Nature. Here we explore what happens to the notion of a black hole in gravity theories where local Lorentz symmetry is violated, and discuss the relevant astrophysical implications. Einstein- aether theory and Ho. rava gravity are used as the theoretical background for addressing this question. We review earlier results about static, spherically symmetric black holes, which demonstrate that in Lorentz- violating theories there can be a new type of horizon and, hence, a new notion of black hole. We also present both known and new results on slowly rotating black holes in these theories, which provide insights on how generic these new horizons are. Finally, we discuss the differences between black holes in Lorentz- violating theories and in General Relativity, and assess to what extent they can be probed with present and future observations.
引用
收藏
页数:22
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