New boundary conditions in Einstein-scalar gravity in three dimensions

被引:2
作者
Anabalon, Andres [1 ]
Gonzalez, Hernan A. [2 ]
Neira-Gallegos, Anibal [3 ]
Oliva, Julio [3 ]
机构
[1] UNESP Univ Estadual Paulista, Inst Fis Teor, R Dr Bento T Ferraz 271,Bl 2, BR-01140070 Sao Paulo, SP, Brazil
[2] Univ San Sebastian, Ave Condor 720, Santiago, Chile
[3] Univ Concepcion, Dept Fis, Casilla 160-C, Concepcion, Chile
基金
巴西圣保罗研究基金会;
关键词
Black Holes; Classical Theories of Gravity; Black Holes in String Theory; ASYMPTOTIC SYMMETRIES; BLACK-HOLES;
D O I
10.1007/JHEP12(2023)149
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We analyze the backreaction of a class of scalar field self-interactions with the possibility of evolving from an AdS vacuum to a fixed point where the scalar field potential vanishes. Exact solutions which interpolate between these regions, ranging from stationary black hole to dynamical spacetimes are constructed. Their surface charges are finite but non-integrable. We study the properties of these charges on the solutions. In particular, we show that the integrable part of the charges provides a realization of the conformal algebra by means of a modification of the Dirac bracket proposed by Barnich and Troessaert. The latter construction allows for a field dependent central extension, whose value tends to the Brown-Henneaux central charge at late times.
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页数:22
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