Light dark matter scattering in gravitational wave detectors

Abstract 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  $$\hbox {GeV}/\text {c}^{2}$$ GeV / c 2 . We investigate how a potential signal compares to typical backgrounds like the...

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Main Authors: Chun-Hao Lee, Chrisna Setyo Nugroho, Martin Spinrath
Format: Article
Language:English
Published: SpringerOpen 2020-12-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-020-08692-3
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author Chun-Hao Lee
Chrisna Setyo Nugroho
Martin Spinrath
author_facet Chun-Hao Lee
Chrisna Setyo Nugroho
Martin Spinrath
author_sort Chun-Hao Lee
collection DOAJ
description Abstract 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  $$\hbox {GeV}/\text {c}^{2}$$ GeV / c 2 . 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.
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spelling doaj.art-e3cc96867bd641cbbfee6ca9251b2af72022-12-21T18:55:08ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-12-01801211610.1140/epjc/s10052-020-08692-3Light dark matter scattering in gravitational wave detectorsChun-Hao Lee0Chrisna Setyo Nugroho1Martin Spinrath2Department of Physics, National Tsing Hua UniversityPhysics Division, National Center for Theoretical SciencesDepartment of Physics, National Tsing Hua UniversityAbstract 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  $$\hbox {GeV}/\text {c}^{2}$$ GeV / c 2 . 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.https://doi.org/10.1140/epjc/s10052-020-08692-3
spellingShingle Chun-Hao Lee
Chrisna Setyo Nugroho
Martin Spinrath
Light dark matter scattering in gravitational wave detectors
European Physical Journal C: Particles and Fields
title Light dark matter scattering in gravitational wave detectors
title_full Light dark matter scattering in gravitational wave detectors
title_fullStr Light dark matter scattering in gravitational wave detectors
title_full_unstemmed Light dark matter scattering in gravitational wave detectors
title_short Light dark matter scattering in gravitational wave detectors
title_sort light dark matter scattering in gravitational wave detectors
url https://doi.org/10.1140/epjc/s10052-020-08692-3
work_keys_str_mv AT chunhaolee lightdarkmatterscatteringingravitationalwavedetectors
AT chrisnasetyonugroho lightdarkmatterscatteringingravitationalwavedetectors
AT martinspinrath lightdarkmatterscatteringingravitationalwavedetectors