Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios

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We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of having SUSY corrections on the ν4→ν γ decay rate, such that the N...

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Detalles Bibliográficos
Autores: Faber T., Liu Y., Porod W., Jones-Pérez J.
Formato: artículo
Fecha de Publicación:2020
Institución:Consejo Nacional de Ciencia Tecnología e Innovación
Repositorio:CONCYTEC-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.concytec.gob.pe:20.500.12390/2574
Enlace del recurso:https://hdl.handle.net/20.500.12390/2574
https://doi.org/10.1103/PhysRevD.101.055029
Nivel de acceso:acceso abierto
Materia:sneutrino
http://purl.org/pe-repo/ocde/ford#2.04.01
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network_name_str CONCYTEC-Institucional
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dc.title.none.fl_str_mv Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
title Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
spellingShingle Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
Faber T.
sneutrino
http://purl.org/pe-repo/ocde/ford#2.04.01
title_short Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
title_full Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
title_fullStr Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
title_full_unstemmed Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
title_sort Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios
author Faber T.
author_facet Faber T.
Liu Y.
Porod W.
Jones-Pérez J.
author_role author
author2 Liu Y.
Porod W.
Jones-Pérez J.
author2_role author
author
author
dc.contributor.author.fl_str_mv Faber T.
Liu Y.
Porod W.
Jones-Pérez J.
dc.subject.none.fl_str_mv sneutrino
topic sneutrino
http://purl.org/pe-repo/ocde/ford#2.04.01
dc.subject.ocde.none.fl_str_mv http://purl.org/pe-repo/ocde/ford#2.04.01
description We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of having SUSY corrections on the ν4→ν γ decay rate, such that the NuStar bounds are relaxed. We find that corrections are too small. For sneutrino dark matter, we consider thermal and nonthermal production, taking into account freeze-out, freeze-in, and super-weakly interacting massive particles mechanisms. For the nonthermal case, we find that the νR can reproduce the observed relic density by adjusting the R-sneutrino mass and Yukawa couplings. For the thermal case, we find the need to extend the model in order to enhance sneutrino annihilations, which we exemplify in a model with an extended gauge symmetry. © 2020 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/" Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.
publishDate 2020
dc.date.accessioned.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.available.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.issued.fl_str_mv 2020
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/2574
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1103/PhysRevD.101.055029
dc.identifier.scopus.none.fl_str_mv 2-s2.0-85083426033
url https://hdl.handle.net/20.500.12390/2574
https://doi.org/10.1103/PhysRevD.101.055029
identifier_str_mv 2-s2.0-85083426033
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv Physical Review D
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.none.fl_str_mv https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/4.0/
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:CONCYTEC-Institucional
instname:Consejo Nacional de Ciencia Tecnología e Innovación
instacron:CONCYTEC
instname_str Consejo Nacional de Ciencia Tecnología e Innovación
instacron_str CONCYTEC
institution CONCYTEC
reponame_str CONCYTEC-Institucional
collection CONCYTEC-Institucional
repository.name.fl_str_mv Repositorio Institucional CONCYTEC
repository.mail.fl_str_mv repositorio@concytec.gob.pe
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spelling Publicationrp02201600rp00930600rp02198600rp02200600Faber T.Liu Y.Porod W.Jones-Pérez J.2024-05-30T23:13:38Z2024-05-30T23:13:38Z2020https://hdl.handle.net/20.500.12390/2574https://doi.org/10.1103/PhysRevD.101.0550292-s2.0-85083426033We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of having SUSY corrections on the ν4→ν γ decay rate, such that the NuStar bounds are relaxed. We find that corrections are too small. For sneutrino dark matter, we consider thermal and nonthermal production, taking into account freeze-out, freeze-in, and super-weakly interacting massive particles mechanisms. For the nonthermal case, we find that the νR can reproduce the observed relic density by adjusting the R-sneutrino mass and Yukawa couplings. For the thermal case, we find the need to extend the model in order to enhance sneutrino annihilations, which we exemplify in a model with an extended gauge symmetry. © 2020 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/" Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - ConcytecengAmerican Physical SocietyPhysical Review Dinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/4.0/sneutrinohttp://purl.org/pe-repo/ocde/ford#2.04.01-1Revisiting neutrino and sneutrino dark matter in natural SUSY scenariosinfo:eu-repo/semantics/articlereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#20.500.12390/2574oai:repositorio.concytec.gob.pe:20.500.12390/25742024-05-30 15:44:11.464https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only accesshttps://repositorio.concytec.gob.peRepositorio Institucional CONCYTECrepositorio@concytec.gob.pe#PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE##PLACEHOLDER_PARENT_METADATA_VALUE#<Publication xmlns="https://www.openaire.eu/cerif-profile/1.1/" id="f4d8800a-6ef3-4e1a-9309-891270d2cc2f"> <Type xmlns="https://www.openaire.eu/cerif-profile/vocab/COAR_Publication_Types">http://purl.org/coar/resource_type/c_1843</Type> <Language>eng</Language> <Title>Revisiting neutrino and sneutrino dark matter in natural SUSY scenarios</Title> <PublishedIn> <Publication> <Title>Physical Review D</Title> </Publication> </PublishedIn> <PublicationDate>2020</PublicationDate> <DOI>https://doi.org/10.1103/PhysRevD.101.055029</DOI> <SCP-Number>2-s2.0-85083426033</SCP-Number> <Authors> <Author> <DisplayName>Faber T.</DisplayName> <Person id="rp02201" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Liu Y.</DisplayName> <Person id="rp00930" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Porod W.</DisplayName> <Person id="rp02198" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Jones-Pérez J.</DisplayName> <Person id="rp02200" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> </Authors> <Editors> </Editors> <Publishers> <Publisher> <DisplayName>American Physical Society</DisplayName> <OrgUnit /> </Publisher> </Publishers> <License>https://creativecommons.org/licenses/by/4.0/</License> <Keyword>sneutrino</Keyword> <Abstract>We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of having SUSY corrections on the ν4→ν γ decay rate, such that the NuStar bounds are relaxed. We find that corrections are too small. For sneutrino dark matter, we consider thermal and nonthermal production, taking into account freeze-out, freeze-in, and super-weakly interacting massive particles mechanisms. For the nonthermal case, we find that the νR can reproduce the observed relic density by adjusting the R-sneutrino mass and Yukawa couplings. For the thermal case, we find the need to extend the model in order to enhance sneutrino annihilations, which we exemplify in a model with an extended gauge symmetry. © 2020 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the &quot;https://creativecommons.org/licenses/by/4.0/&quot; Creative Commons Attribution 4.0 International license. 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