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Simple Hidden Sector Dark Matter

A hidden sector that kinetically mixes with the minimal supersymmetric standard model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP). These supersymmetric constructions can also provide a natur...

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Detalles Bibliográficos
Autores principales: Barnes, Patrick, Johnson, Zachary, Pierce, Aaron, Shakya, Bibhushan
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.102.075019
http://cds.cern.ch/record/2714529
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author Barnes, Patrick
Johnson, Zachary
Pierce, Aaron
Shakya, Bibhushan
author_facet Barnes, Patrick
Johnson, Zachary
Pierce, Aaron
Shakya, Bibhushan
author_sort Barnes, Patrick
collection CERN
description A hidden sector that kinetically mixes with the minimal supersymmetric standard model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP). These supersymmetric constructions can also provide a natural explanation for why the dark matter is at the weak scale even if it resides in a hidden sector. In the hidden sector, a natural pattern of symmetry breaking generally makes particles and their superpartners lie around the same mass scale, opening novel possibilities for a variety of cosmological histories and complex indirect detection signatures.
id cern-2714529
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
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spelling cern-27145292022-08-23T02:06:16Zdoi:10.1103/PhysRevD.102.075019http://cds.cern.ch/record/2714529engBarnes, PatrickJohnson, ZacharyPierce, AaronShakya, BibhushanSimple Hidden Sector Dark Matterastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyA hidden sector that kinetically mixes with the minimal supersymmetric standard model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP). These supersymmetric constructions can also provide a natural explanation for why the dark matter is at the weak scale even if it resides in a hidden sector. In the hidden sector, a natural pattern of symmetry breaking generally makes particles and their superpartners lie around the same mass scale, opening novel possibilities for a variety of cosmological histories and complex indirect detection signatures.A hidden sector that kinetically mixes with the Minimal Supersymmetric Standard Model provides simple and well-motivated dark matter candidates that possess many of the properties of a traditional weakly interacting massive particle (WIMP). These supersymmetric constructions can also provide a natural explanation for why the dark matter is at the weak scale - even if it resides in a hidden sector. In the hidden sector, a natural pattern of symmetry breaking generally makes particles and their superpartners lie around the same mass scale, opening novel possibilities for a variety of cosmological histories and complex indirect detection signatures.arXiv:2003.13744LCTP-20-05CERN-TH-2020-024oai:cds.cern.ch:27145292020-03-30
spellingShingle astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Barnes, Patrick
Johnson, Zachary
Pierce, Aaron
Shakya, Bibhushan
Simple Hidden Sector Dark Matter
title Simple Hidden Sector Dark Matter
title_full Simple Hidden Sector Dark Matter
title_fullStr Simple Hidden Sector Dark Matter
title_full_unstemmed Simple Hidden Sector Dark Matter
title_short Simple Hidden Sector Dark Matter
title_sort simple hidden sector dark matter
topic astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.102.075019
http://cds.cern.ch/record/2714529
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AT johnsonzachary simplehiddensectordarkmatter
AT pierceaaron simplehiddensectordarkmatter
AT shakyabibhushan simplehiddensectordarkmatter