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Strongly Interacting Light Dark Matter

In the presence of approximate global symmetries that forbid relevantinteractions, strongly coupled light Dark Matter (DM) can appear weakly coupledat small energy and generate a sizable relic abundance. Fundamental principleslike unitarity restrict these symmetries to a small class, where the leadi...

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Detalles Bibliográficos
Autores principales: Bruggisser, Sebastian, Riva, Francesco, Urbano, Alfredo
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.21468/SciPostPhys.3.3.017
http://cds.cern.ch/record/2198106
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author Bruggisser, Sebastian
Riva, Francesco
Urbano, Alfredo
author_facet Bruggisser, Sebastian
Riva, Francesco
Urbano, Alfredo
author_sort Bruggisser, Sebastian
collection CERN
description In the presence of approximate global symmetries that forbid relevantinteractions, strongly coupled light Dark Matter (DM) can appear weakly coupledat small energy and generate a sizable relic abundance. Fundamental principleslike unitarity restrict these symmetries to a small class, where the leadinginteractions are captured by effective operators up to dimension-8. Chiralsymmetry, spontaneously broken global symmetries and non-linearly realizedsupersymmetry are examples of this. Their DM candidates (composite fermions,pseudo Nambu-Goldstone Bosons and Goldstini) are interesting targets for LHCmissing-energy searches.
id cern-2198106
institution Organización Europea para la Investigación Nuclear
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publishDate 2016
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spelling cern-21981062023-03-14T19:35:33Zdoi:10.21468/SciPostPhys.3.3.017http://cds.cern.ch/record/2198106engBruggisser, SebastianRiva, FrancescoUrbano, AlfredoStrongly Interacting Light Dark Matterhep-thParticle Physics - Theoryhep-phParticle Physics - PhenomenologyIn the presence of approximate global symmetries that forbid relevantinteractions, strongly coupled light Dark Matter (DM) can appear weakly coupledat small energy and generate a sizable relic abundance. Fundamental principleslike unitarity restrict these symmetries to a small class, where the leadinginteractions are captured by effective operators up to dimension-8. Chiralsymmetry, spontaneously broken global symmetries and non-linearly realizedsupersymmetry are examples of this. Their DM candidates (composite fermions,pseudo Nambu-Goldstone Bosons and Goldstini) are interesting targets for LHCmissing-energy searches.In the presence of approximate global symmetries that forbid relevant interactions, strongly coupled light Dark Matter (DM) can appear weakly coupled at small energy and generate a sizable relic abundance. Fundamental principles like unitarity restrict these symmetries to a small class, where the leading interactions are captured by effective operators up to dimension-8. Chiral symmetry, spontaneously broken global symmetries and non-linearly realized supersymmetry are examples of this. Their DM candidates (composite fermions, pseudo Nambu-Goldstone Bosons and Goldstini) are interesting targets for LHC missing-energy searches.arXiv:1607.02474DESY-16-122CERN-TH-2016-153oai:cds.cern.ch:21981062016-07-08
spellingShingle hep-th
Particle Physics - Theory
hep-ph
Particle Physics - Phenomenology
Bruggisser, Sebastian
Riva, Francesco
Urbano, Alfredo
Strongly Interacting Light Dark Matter
title Strongly Interacting Light Dark Matter
title_full Strongly Interacting Light Dark Matter
title_fullStr Strongly Interacting Light Dark Matter
title_full_unstemmed Strongly Interacting Light Dark Matter
title_short Strongly Interacting Light Dark Matter
title_sort strongly interacting light dark matter
topic hep-th
Particle Physics - Theory
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.21468/SciPostPhys.3.3.017
http://cds.cern.ch/record/2198106
work_keys_str_mv AT bruggissersebastian stronglyinteractinglightdarkmatter
AT rivafrancesco stronglyinteractinglightdarkmatter
AT urbanoalfredo stronglyinteractinglightdarkmatter