Exploring dark forces with multimessenger studies of extreme mass ratio inspirals

被引：1

作者：

Bhalla, Badal ^{[1
]}

Sinha, Kuver ^{[1
]}

Xu, Tao ^{[1
]}

机构：

[1] Univ Oklahoma, Homer L Dodge Dept Phys & Astron, Norman, OK 73019 USA

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2024年 / 09期

关键词：

astrophysical black holes; gravitational waves / sources; massive black holes; BLACK-HOLE; GRAVITATIONAL-WAVES; TESTS;

D O I：

10.1088/1475-7516/2024/09/023

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The exploration of dark sector interactions via gravitational waves (GWs) from binary inspirals has been a subject of recent interest. We study dark forces using extreme mass ratio inspirals (EMRIs), pointing out two issues of interest. Firstly, the innermost stable circular orbit (ISCO) of the EMRI, which sets the characteristic length scale of the system and hence the dark force range to which it exhibits enhanced sensitivity, probes force mediator masses that complement those studied with supermassive black hole (SMBH) or neutron star binaries. The LISA mission (the proposed mu Ares detector) will probe mediators with masses m(V) similar to 10(-16) eV (m(V) similar to 10(-18) eV), corresponding to ISCOs of 10(6)M(circle dot) (10(8)M(circle dot)) central SMBHs. Secondly, while the sensitivity to dark couplings is typically limited by the uncertainty in the binary component masses, independent mass measurements of the central SMBH through reverberation mapping campaigns or the motion of dynamical tracers enable one to break this degeneracy. Our results therefore highlight the necessity for coordinated studies, loosely referred to as "multimessenger", between future mu Hz- mHz GW observatories and ongoing and forthcoming SMBH mass measurement campaigns, including OzDES-RM, SDSS-RM, and SDSS-V Black Hole Mapper.

引用

页数：27

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