Rotating black holes embedded in a cosmological background for scalar-tensor theories

被引：4
作者：
Babichev, Eugeny [1 ]
Charmousis, Christos [1 ]
Lecoeur, Nicolas [1 ]
机构：
[1] Univ Paris Saclay, IJCLab, CNRS, IN2P3, F-91405 Orsay, France
来源：
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2023年 / 08期
关键词：
Sitter spacetimes; Exact solutions; black holes and black hole thermodynamics in GR and beyond; Gauss-Bonnet-Lovelock-Horndeski-Palatini etc gravity theories; modified gravity; DARK ENERGY; ACCRETION; MASS;
D O I：
10.1088/1475-7516/2023/08/022
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present solutions of DHOST theories describing a rotating black hole embedded in an expanding universe. The solution is constructed by conformal transformation of a stealth Kerr(-de Sitter) black hole. The conformal factor depends explicitly on the scalar field - but not on its derivative - and defines the new theory. The scalar field of the stealth Kerr(-de Sitter) solution depends on time, leading to the time-dependence of the obtained conformal metric, with cosmological asymptotics at large distances. We study the properties of the obtained metric by considering regular null geodesic congruences, and identify trapping black hole and cosmological horizons.
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页数：34
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