Testing gravity of a disformal Kerr black hole in quadratic degenerate higher-order scalar-tensor theories by quasi-periodic oscillations

被引：13

作者：

Chen, Songbai ^{[1
,2
]}

Wang, Zejun ^{[1
]}

Jing, Jiliang ^{[1
,2
]}

机构：

[1] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Dept Phys,Minist Educ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Changsha 410081, Hunan, Peoples R China

[2] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2021年 / 06期

基金：

中国国家自然科学基金;

关键词：

GR black holes; modified gravity; X-RAY BINARIES; MASS; PRECESSION;

D O I：

10.1088/1475-7516/2021/06/043

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

By using the relativistic precession model, we have studied frequencies of quasiperiodic oscillations in the spacetime of a disformal Kerr black hole. This black hole owns an extra disformal parameter and belongs to a class of non-stealth solutions in quadratic degenerate higher-order scalar-tensor (DHOST) theories. Our result shows that only the periastron precession frequency is related to the disformal parameter, while the azimuthal frequency and the nodal precession frequency are identical with those in the usual Kerr black hole in general relativity. Combing with the observation data of GRO J1655-40, we fit parameters of the disformal Kerr black hole, and find that the disformal parameter alpha is almost negative in the range of 1 sigma, which implies the negative disformal parameter alpha is favored by the observation data of GRO J1655-40.

引用

页数：12

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