Yayın:
Naturalness and Dark Matter Properties of the BLSSM

dc.contributor.authorRose, L.D.
dc.contributor.authorKhalil, S.
dc.contributor.authorKing, S.
dc.contributor.authorMarzo, C.
dc.contributor.authorMoretti, S.
dc.contributor.authorÜn, C.S.
dc.contributor.buuauthorÜN, CEM SALİH
dc.contributor.departmentFen Edebiyat Fakültesi
dc.contributor.departmentFizik Ana Bilim Dalı
dc.contributor.orcid0000-0002-0595-8803
dc.contributor.scopusid55325758100
dc.date.accessioned2025-08-06T23:06:24Z
dc.date.issued2017-01-01
dc.description.abstractIn this report, we compare the naturalness and Dark Matter (DM) properties of the Minimal Supersymmetric Standard Model (MSSM) and the B-L Supersymmetric Standard Model (BLSSM), with universality in both cases. We do this by adopting standard measures for the quantitative analysis of the Fine-Tuning (FT), at both low (i.e. supersymmetric (SUSY)) and high (i.e. unification) scales. We will see a similar level of FT for both models in these scenarios, with a slightly better FT for the BLSSM at SUSY scales and MSSM at Grand Unification Theory (GUT) scales. When includingDMrelic constraints, we drastically confine the MSSM's parameter space, whereas we still find a large parameter space available for the non-minimal scenario.
dc.identifier.scopus2-s2.0-85041651838
dc.identifier.urihttps://hdl.handle.net/11452/53643
dc.identifier.volume2017-April
dc.indexed.scopusScopus
dc.language.isoen
dc.publisherSissa Medialab Srl
dc.relation.journalProceedings of Science
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subject.scopusSupersymmetry and Dark Matter in Particle Physics
dc.titleNaturalness and Dark Matter Properties of the BLSSM
dc.typeconferenceObject
dc.type.subtypeConference Paper
dspace.entity.typePublication
local.contributor.departmentFen Edebiyat Fakültesi/ Fizik Ana Bilim Dalı
local.indexed.atScopus
relation.isAuthorOfPublication0c6ad07c-f6f6-4949-a2f0-e288af6b9411
relation.isAuthorOfPublication.latestForDiscovery0c6ad07c-f6f6-4949-a2f0-e288af6b9411

Dosyalar