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dc.date.accessioned 2021-09-23T15:15:31Z
dc.date.available 2021-09-23T15:15:31Z
dc.date.issued 2021-04-01
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/125491
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. en
dc.language en es
dc.subject New Physics es
dc.subject Supersymmetry es
dc.subject Dark Matter es
dc.subject Sneutrino es
dc.title Dark matter candidates in the NMSSM with RH neutrino superfields en
dc.type Articulo es
sedici.identifier.other arXiv:2102.08986 es
sedici.identifier.other doi:10.1088/1475-7516/2021/04/067 es
sedici.identifier.issn 1475-7516 es
sedici.creator.person López-Fogliani, Daniel E. es
sedici.creator.person Pérez, Andrés Daniel es
sedici.creator.person de Austri, Roberto Ruiz es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Journal of Cosmology and Astroparticle Physics es
sedici.relation.journalVolumeAndIssue vol. 2021, no. 4 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)