Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor

Abstract We study the gravitational waves (GWs) spectrum produced during the electroweak phase transition in a scale-invariant extension of the Standard Model (SM), enlarged by a dark $$ U(1)_{D} $$ U(1)D gauge symmetry. This symmetry incorporates a vector dark matter (DM) candidate and a scalar fie...

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Main Author: Ahmad Mohamadnejad
Format: Article
Language:English
Published: SpringerOpen 2020-03-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-7756-6
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spelling doaj-7647c5c72aae400dbf013d01749a2d5d2020-11-24T21:41:56ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-03-0180311310.1140/epjc/s10052-020-7756-6Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floorAhmad Mohamadnejad0Department of Physics, Lorestan UniversityAbstract We study the gravitational waves (GWs) spectrum produced during the electroweak phase transition in a scale-invariant extension of the Standard Model (SM), enlarged by a dark $$ U(1)_{D} $$ U(1)D gauge symmetry. This symmetry incorporates a vector dark matter (DM) candidate and a scalar field (scalon). Because of scale invariance, the model has only two independent parameters and for the parameter space constrained by DM relic density, strongly first-order electroweak phase transition can take place. In this model, for a narrow part of the parameter space, DM-nucleon cross section is below the neutrino-floor limit, and therefore, it cannot be probed by the future direct detection experiments. However, for a benchmark point from this narrow region, we show the amplitude and frequency of phase transition GW spectrum fall within the observational window of space-based GW detectors such as eLISA.http://link.springer.com/article/10.1140/epjc/s10052-020-7756-6
collection DOAJ
language English
format Article
sources DOAJ
author Ahmad Mohamadnejad
spellingShingle Ahmad Mohamadnejad
Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
European Physical Journal C: Particles and Fields
author_facet Ahmad Mohamadnejad
author_sort Ahmad Mohamadnejad
title Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
title_short Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
title_full Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
title_fullStr Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
title_full_unstemmed Gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
title_sort gravitational waves from scale-invariant vector dark matter model: probing below the neutrino-floor
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2020-03-01
description Abstract We study the gravitational waves (GWs) spectrum produced during the electroweak phase transition in a scale-invariant extension of the Standard Model (SM), enlarged by a dark $$ U(1)_{D} $$ U(1)D gauge symmetry. This symmetry incorporates a vector dark matter (DM) candidate and a scalar field (scalon). Because of scale invariance, the model has only two independent parameters and for the parameter space constrained by DM relic density, strongly first-order electroweak phase transition can take place. In this model, for a narrow part of the parameter space, DM-nucleon cross section is below the neutrino-floor limit, and therefore, it cannot be probed by the future direct detection experiments. However, for a benchmark point from this narrow region, we show the amplitude and frequency of phase transition GW spectrum fall within the observational window of space-based GW detectors such as eLISA.
url http://link.springer.com/article/10.1140/epjc/s10052-020-7756-6
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