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From NANOGrav to LIGO with metastable cosmic strings

We interpret the recent NANOGrav results in terms of a stochastic gravitational wave background from metastable cosmic strings. The observed amplitude of a stochastic signal can be translated into a range for the cosmic string tension and the mass of magnetic monopoles arising in theories of grand u...

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Detalles Bibliográficos
Autores principales: Buchmuller, Wilfried, Domcke, Valerie, Schmitz, Kai
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2020.135914
http://cds.cern.ch/record/2732057
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author Buchmuller, Wilfried
Domcke, Valerie
Schmitz, Kai
author_facet Buchmuller, Wilfried
Domcke, Valerie
Schmitz, Kai
author_sort Buchmuller, Wilfried
collection CERN
description We interpret the recent NANOGrav results in terms of a stochastic gravitational wave background from metastable cosmic strings. The observed amplitude of a stochastic signal can be translated into a range for the cosmic string tension and the mass of magnetic monopoles arising in theories of grand unification. In a sizable part of the parameter space, this interpretation predicts a large stochastic gravitational wave signal in the frequency band of ground-based interferometers, which can be probed in the very near future. We confront these results with predictions from successful inflation, leptogenesis and dark matter from the spontaneous breaking of a gauged B − L symmetry.
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spelling cern-27320572023-10-04T06:40:09Zdoi:10.1016/j.physletb.2020.135914http://cds.cern.ch/record/2732057engBuchmuller, WilfriedDomcke, ValerieSchmitz, KaiFrom NANOGrav to LIGO with metastable cosmic stringshep-phParticle Physics - Phenomenologyastro-ph.COAstrophysics and AstronomyWe interpret the recent NANOGrav results in terms of a stochastic gravitational wave background from metastable cosmic strings. The observed amplitude of a stochastic signal can be translated into a range for the cosmic string tension and the mass of magnetic monopoles arising in theories of grand unification. In a sizable part of the parameter space, this interpretation predicts a large stochastic gravitational wave signal in the frequency band of ground-based interferometers, which can be probed in the very near future. We confront these results with predictions from successful inflation, leptogenesis and dark matter from the spontaneous breaking of a gauged B − L symmetry.We interpret the recent NANOGrav results in terms of a stochastic gravitational wave background from metastable cosmic strings. The observed amplitude of a stochastic signal can be translated into a range for the cosmic string tension and the mass of magnetic monopoles arising in theories of grand unification. In a sizable part of the parameter space, this interpretation predicts a large stochastic gravitational wave signal in the frequency band of ground-based interferometers, which can be probed in the very near future. We confront these results with predictions from successful inflation, leptogenesis and dark matter from the spontaneous breaking of a gauged B-L symmetry.arXiv:2009.10649CERN-TH-2020-157DESY 20-154DESY-20-154oai:cds.cern.ch:27320572020-09-22
spellingShingle hep-ph
Particle Physics - Phenomenology
astro-ph.CO
Astrophysics and Astronomy
Buchmuller, Wilfried
Domcke, Valerie
Schmitz, Kai
From NANOGrav to LIGO with metastable cosmic strings
title From NANOGrav to LIGO with metastable cosmic strings
title_full From NANOGrav to LIGO with metastable cosmic strings
title_fullStr From NANOGrav to LIGO with metastable cosmic strings
title_full_unstemmed From NANOGrav to LIGO with metastable cosmic strings
title_short From NANOGrav to LIGO with metastable cosmic strings
title_sort from nanograv to ligo with metastable cosmic strings
topic hep-ph
Particle Physics - Phenomenology
astro-ph.CO
Astrophysics and Astronomy
url https://dx.doi.org/10.1016/j.physletb.2020.135914
http://cds.cern.ch/record/2732057
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