Light dark matter scattering in gravitational wave detectors

被引：7

作者：

Lee, Chun-Hao ^{[1
]}

Nugroho, Chrisna Setyo ^{[2
]}

Spinrath, Martin ^{[1
]}

机构：

[1] Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan

[2] Natl Ctr Theoret Sci, Phys Div, Hsinchu 30013, Taiwan

来源：

EUROPEAN PHYSICAL JOURNAL C | 2020年 / 80卷 / 12期

关键词：

THERMAL NOISE;

D O I：

10.1140/epjc/s10052-020-08692-3

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 present prospects for discovering dark matter scattering in gravitational wave detectors. The focus of this work is on light, particle dark matter with masses below 1 GeV/c2. We investigate how a potential signal compares to typical backgrounds like thermal and quantum noise, first in a simple toy model and then using KAGRA as a realistic example. That shows that for a discovery much lighter and cooler mirrors would be needed. We also give some brief comments on space-based experiments and future atomic interferometers.

引用

页数：16

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