Carroll black holes

被引:27
作者
Ecker, Florian [1 ]
Grumiller, Daniel [1 ,2 ]
Hartong, Jelle [3 ,4 ]
Perez, Alfredo [5 ,6 ]
Prohazka, Stefan [3 ,4 ]
Troncoso, Ricardo [5 ,6 ]
机构
[1] TU Wien, Inst Theoret Phys, Wiedner Hauptstr 8-10, A-1040 Vienna, Austria
[2] Okinawa Inst Sci & Technol Grad Univ, Theoret Sci Visiting Program, Onna 9040495, Japan
[3] Univ Edinburgh, Sch Math, Peter Guthrie Tait Rd, Edinburgh EH9 3FD, Scotland
[4] Univ Edinburgh, Maxwell Inst Math Sci, Peter Guthrie Tait Rd, Edinburgh EH9 3FD, Scotland
[5] Ctr Estudios Cient, Ave Arturo Prat 514, Valdivia, Chile
[6] Univ San Sebastian, Fac Ingn Arquitectura & Diseno, Gen Lagos 1163, Valdivia 5110693, Chile
基金
奥地利科学基金会;
关键词
GAUGE-THEORY; CLASSICAL-SOLUTIONS; GRAVITY; FIELD; DIMENSIONS;
D O I
10.21468/SciPostPhys.15.6.245
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Despite the absence of a lightcone structure, some solutions of Carroll gravity show black hole-like behaviour. We define Carroll black holes as solutions of Carroll gravity that ex-hibit Carroll thermal properties and have a Carroll extremal surface, notions introduced in our work. The latter is a Carroll analogue of a Lorentzian extremal surface. As ex-amples, we discuss the Carroll versions of Schwarzschild, Reissner-Nordstrom, and BTZ black holes and black hole solutions of generic 1+1 dimensional Carroll dilaton gravity, including Carroll JT and Carroll Witten black holes.
引用
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页数:59
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