Boundary causality versus hyperbolicity for spherical black holes in Gauss-Bonnet gravity

被引:13
作者
Andrade, Tomas [1 ]
Caceres, Elena [2 ,3 ]
Keeler, Cynthia [4 ]
机构
[1] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, 1 Keble Rd, Oxford OX1 3NP, England
[2] Univ Colima, Fac Ciencias, Bernal Diaz del Castillo 340, Colima, Mexico
[3] Univ Texas Austin, Dept Phys, Theory Grp, Austin, TX 78712 USA
[4] Univ Copenhagen, Niels Bohr Int Acad, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
基金
美国国家科学基金会; 欧洲研究理事会; 新加坡国家研究基金会;
关键词
Gauss-Bonnet gravity; higher curvature gravity; hyperbolicity; causality; THERMODYNAMICS;
D O I
10.1088/1361-6382/aa7101
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We explore the constraints boundary causality places on the allowable Gauss-Bonnet gravitational couplings in asymptotically AdS spaces, specifically considering spherical black hole solutions. We additionally consider the hyperbolicity properties of these solutions, positing that hyperbolicityviolating solutions are sick solutions whose causality properties provide no information about the theory they reside in. For both signs of the Gauss-Bonnet coupling, spherical black holes violate boundary causality at smaller absolute values of the coupling than planar black holes do. For negative coupling, as we tune the Gauss-Bonnet coupling away from zero, both spherical and planar black holes violate hyperbolicity before they violate boundary causality. For positive coupling, the only hyperbolicity-respecting spherical black holes which violate boundary causality do not do so appreciably far from the planar bound. Consequently, eliminating hyperbolicity-violating solutions means the bound on Gauss-Bonnet couplings from the boundary causality of spherical black holes is no tighter than that from planar black holes.
引用
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页数:16
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