Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves

Fuente: arXiv
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1. Verfasser: Xu, Yong
Format: Preprint
Veröffentlicht: 2024
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author Xu, Yong
author_facet Xu, Yong
contents The evidence for the existence of dark matter (DM) is compelling, yet its nature remains elusive. A minimal scenario involves DM interacting solely through gravity. However, the detection would be extremely challenging. In the early Universe, such DM can be unavoidably generated via annihilation of particles in the standard model (SM) thermal plasma. It is known that the SM thermal plasma also produces gravitational waves (GWs). In this study, we establish a simple connection between the amplitude of thermal GWs and the properties of pure gravitational DM. Notably, future GW experiments in the ultra-high frequency regime have the potential to shed light on the mass and spin of pure gravitational DM.
format Preprint
id arxiv_https___arxiv_org_abs_2412_21137
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves
Xu, Yong
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
The evidence for the existence of dark matter (DM) is compelling, yet its nature remains elusive. A minimal scenario involves DM interacting solely through gravity. However, the detection would be extremely challenging. In the early Universe, such DM can be unavoidably generated via annihilation of particles in the standard model (SM) thermal plasma. It is known that the SM thermal plasma also produces gravitational waves (GWs). In this study, we establish a simple connection between the amplitude of thermal GWs and the properties of pure gravitational DM. Notably, future GW experiments in the ultra-high frequency regime have the potential to shed light on the mass and spin of pure gravitational DM.
title Probing Gravitational Dark Matter with Ultra-high Frequency Gravitational Waves
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2412.21137