WIMP dark matter in the U μνSSM
- Autores
- Aguilar Saavedra, J. A.; Lopez, Daniel Elbio; Muñoz, C.; Pierre, M.
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The UμνSSM is a U(1)' extension of the μνSSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of UμνSSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete Z 2 symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking R-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via Z', Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to Z'; direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment.
Fil: Aguilar Saavedra, J. A.. Universidad de Granada; España. Consejo Superior de Investigaciones Científicas; España
Fil: Lopez, Daniel Elbio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Pontificia Universidad Católica Argentina "Santa María de los Buenos Aires"; Argentina
Fil: Muñoz, C.. Universidad Autónoma de Madrid; España
Fil: Pierre, M.. Universidad Autónoma de Madrid; España - Materia
-
DARK MATTER THEORY
PARTICLE PHYSICS - COSMOLOGY CONNECTION
SUPERSYMMETRY AND COSMOLOGY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/214236
Ver los metadatos del registro completo
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WIMP dark matter in the U μνSSMAguilar Saavedra, J. A.Lopez, Daniel ElbioMuñoz, C.Pierre, M.DARK MATTER THEORYPARTICLE PHYSICS - COSMOLOGY CONNECTIONSUPERSYMMETRY AND COSMOLOGYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The UμνSSM is a U(1)' extension of the μνSSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of UμνSSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete Z 2 symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking R-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via Z', Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to Z'; direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment.Fil: Aguilar Saavedra, J. A.. Universidad de Granada; España. Consejo Superior de Investigaciones Científicas; EspañaFil: Lopez, Daniel Elbio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Pontificia Universidad Católica Argentina "Santa María de los Buenos Aires"; ArgentinaFil: Muñoz, C.. Universidad Autónoma de Madrid; EspañaFil: Pierre, M.. Universidad Autónoma de Madrid; EspañaIOP Publishing2022-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/214236Aguilar Saavedra, J. A.; Lopez, Daniel Elbio; Muñoz, C.; Pierre, M.; WIMP dark matter in the U μνSSM; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2022; 5; 5-2022; 1-311475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2022/05/004info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2022/05/004info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:06:51Zoai:ri.conicet.gov.ar:11336/214236instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:06:52.115CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
WIMP dark matter in the U μνSSM |
title |
WIMP dark matter in the U μνSSM |
spellingShingle |
WIMP dark matter in the U μνSSM Aguilar Saavedra, J. A. DARK MATTER THEORY PARTICLE PHYSICS - COSMOLOGY CONNECTION SUPERSYMMETRY AND COSMOLOGY |
title_short |
WIMP dark matter in the U μνSSM |
title_full |
WIMP dark matter in the U μνSSM |
title_fullStr |
WIMP dark matter in the U μνSSM |
title_full_unstemmed |
WIMP dark matter in the U μνSSM |
title_sort |
WIMP dark matter in the U μνSSM |
dc.creator.none.fl_str_mv |
Aguilar Saavedra, J. A. Lopez, Daniel Elbio Muñoz, C. Pierre, M. |
author |
Aguilar Saavedra, J. A. |
author_facet |
Aguilar Saavedra, J. A. Lopez, Daniel Elbio Muñoz, C. Pierre, M. |
author_role |
author |
author2 |
Lopez, Daniel Elbio Muñoz, C. Pierre, M. |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
DARK MATTER THEORY PARTICLE PHYSICS - COSMOLOGY CONNECTION SUPERSYMMETRY AND COSMOLOGY |
topic |
DARK MATTER THEORY PARTICLE PHYSICS - COSMOLOGY CONNECTION SUPERSYMMETRY AND COSMOLOGY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The UμνSSM is a U(1)' extension of the μνSSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of UμνSSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete Z 2 symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking R-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via Z', Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to Z'; direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment. Fil: Aguilar Saavedra, J. A.. Universidad de Granada; España. Consejo Superior de Investigaciones Científicas; España Fil: Lopez, Daniel Elbio. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina. Pontificia Universidad Católica Argentina "Santa María de los Buenos Aires"; Argentina Fil: Muñoz, C.. Universidad Autónoma de Madrid; España Fil: Pierre, M.. Universidad Autónoma de Madrid; España |
description |
The UμνSSM is a U(1)' extension of the μνSSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of UμνSSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete Z 2 symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking R-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via Z', Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to Z'; direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-05 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/214236 Aguilar Saavedra, J. A.; Lopez, Daniel Elbio; Muñoz, C.; Pierre, M.; WIMP dark matter in the U μνSSM; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2022; 5; 5-2022; 1-31 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/214236 |
identifier_str_mv |
Aguilar Saavedra, J. A.; Lopez, Daniel Elbio; Muñoz, C.; Pierre, M.; WIMP dark matter in the U μνSSM; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2022; 5; 5-2022; 1-31 1475-7516 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2022/05/004 info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2022/05/004 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.070432 |