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dc.contributor.author
López Fogliani, Daniel E.  
dc.contributor.author
Perez, Andres Daniel  
dc.contributor.author
Ruiz de Austri, Roberto  
dc.date.available
2022-12-14T14:57:59Z  
dc.date.issued
2021-04  
dc.identifier.citation
López Fogliani, Daniel E.; Perez, Andres Daniel; Ruiz de Austri, Roberto; Dark matter candidates in the NMSSM with RH neutrino superfields; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2021; 4; 4-2021; 1-36  
dc.identifier.issn
1475-7516  
dc.identifier.uri
http://hdl.handle.net/11336/181133  
dc.description.abstract
R-parity conserving supersymmetric models with right-handed (RH) neutrinos are very appealing since they could naturally explain neutrino physics and also provide a good dark matter (DM) candidate such as the lightest supersymmetric particle (LSP). In this work we consider the next-to-minimal supersymmetric standard model (NMSSM) plus RH neutrino superfields, with effective Majorana masses dynamically generated at the electroweak scale (EW). We perform a scan of the relevant parameter space and study both possible DM candidates: RH sneutrino and neutralino. Especially for the case of RH sneutrino DM we analyse the intimate relation between both candidates to obtain the correct amount of relic density. Besides the well-known resonances, annihilations through scalar quartic couplings and coannihilation mechanisms with all kind of neutralinos, are crucial. Finally, we present the impact of current and future direct and indirect detection experiments on both DM candidates.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
IOP Publishing  
dc.rights
info:eu-repo/semantics/restrictedAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
DARK MATTER DETECTORS  
dc.subject
DARK MATTER THEORY  
dc.subject.classification
Física de Partículas y Campos  
dc.subject.classification
Ciencias Físicas  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Dark matter candidates in the NMSSM with RH neutrino superfields  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2022-09-20T15:47:26Z  
dc.journal.volume
2021  
dc.journal.number
4  
dc.journal.pagination
1-36  
dc.journal.pais
Reino Unido  
dc.journal.ciudad
Londres  
dc.description.fil
Fil: López Fogliani, Daniel E.. 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  
dc.description.fil
Fil: Perez, Andres Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina  
dc.description.fil
Fil: Ruiz de Austri, Roberto. Consejo Superior de Investigaciones Científicas; España. Universidad de Valencia; España. Instituto de Física Corpuscular; España  
dc.journal.title
Journal of Cosmology and Astroparticle Physics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2021/04/067  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1088/1475-7516/2021/04/067