Dressed black holes in the new tensor-vector-scalar theory

被引:10
作者
Bernardo, Reginald Christian [1 ]
Chen, Che-Yu [1 ]
机构
[1] Acad Sinica, Inst Phys, Taipei 11529, Taiwan
关键词
Black holes; No-hair theorem; Alternative gravity; Modified Newtonian dynamics; NEWTONIAN DYNAMICS; SHADOW; MASS;
D O I
10.1007/s10714-023-03075-x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
As incarnations of gravity in its prime, black holes are arguably the best target for us to demystify gravity. Keeping in mind the prominent role black holes play in gravitational wave astronomy, it becomes a must for a theory to possess black hole solutions with only measurable departures from their general relativity counterparts. In this paper, we present black holes in a tensor-vector-scalar representation of relativistic modified Newtonian dynamics. We find that the theory allows Schwarzschild and nearly-Schwarzschild black holes as solutions, while the nontrivial scalar and vector fields generally diverge at the event horizon. Whether this is a physical pathology or not poses a challenge for these solutions, and by extension, the model. However, even if it is, this pathology could be overcome when the black hole hair vanishes.
引用
收藏
页数:29
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