New probe of dark matter-induced fifth force with neutron star inspirals

被引：18
作者：
Choi, Han Gil [1 ]
Jung, Sunghoon [1 ]
机构：
[1] Seoul Natl Univ, Dept Phys & Astron, Ctr Theoret Phys, Seoul 08826, South Korea
来源：
PHYSICAL REVIEW D | 2019年 / 99卷 / 01期
基金：
新加坡国家研究基金会;
关键词：
GRAVITATIONAL-WAVES; PULSAR;
D O I：
10.1103/PhysRevD.99.015013
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A light scalar dark matter (DM) is allowed in a wide range of its mass and interaction types. We show that the light scalar DM may be probed in a new way from final years of neutron-star (NS) binary inspirals. If the DM interacts with the neutron, its long wave coherence in the background can induce the time-oscillating mass shift, to which the binary inspiral is inherently sensitive, but the sensitivity is found to be significantly enhanced by a large number of gravitational-wave (GW) cycles during year-long highest-frequency measurements in the broadband f similar or equal to 0.01-1000 Hz. Such broadband measurements that can be realized by a future detector network including LIGO and mid-band detectors can probe unconstrained parameter space of the light scalar DM.
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页数：11
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