Publication: Prospects for sneutrino dark matter in the blssm
dc.contributor.author | King, Simon J. D. | |
dc.contributor.author | Delle Rose, Luigi | |
dc.contributor.author | Khalil, Shaaban | |
dc.contributor.author | Kulkarni, Suchita | |
dc.contributor.author | Marzo, Carlo | |
dc.contributor.author | Moretti, Stefano | |
dc.contributor.buuauthor | Ün, Cem Salih | |
dc.contributor.buuauthor | ÜN, CEM SALİH | |
dc.contributor.department | Bursa Uludağ Üniversitesi/Fen Edebiyat Fakültesi/Fizik Anabilim Dalı. | |
dc.contributor.researcherid | N-3421-2014 | |
dc.date.accessioned | 2024-11-07T11:21:23Z | |
dc.date.available | 2024-11-07T11:21:23Z | |
dc.date.issued | 2018-07-01 | |
dc.description.abstract | The (B - L) Supersymmetric Standard Model (BLSSM) motivates several Dark Matter (DM) candidates beyond the Minimally Supersymmetric Standard Model (MSSM). We assess the comparative naturalness of the two models and discuss the potential detection properties of a particular candidate, the Right-Handed (RH) sneutrino. | |
dc.description.sponsorship | NExT Institute | |
dc.description.sponsorship | STFC/COFUND Rutherford International Fellowship scheme | |
dc.description.sponsorship | "Angelo Della Riccia" foundation | |
dc.description.sponsorship | Centre of Excellence project "Dark Side of the Universe" TK133 | |
dc.description.sponsorship | Science and Technology Development Fund (STDF) 13858 | |
dc.description.sponsorship | H2020-MSCA-RISE-2014 645722 | |
dc.description.sponsorship | UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) ST/L000296/1 | |
dc.description.sponsorship | "New Frontiers" program of the Austrian Academy of Sciences | |
dc.description.sponsorship | Austrian Science Fund (FWF) V592-N27 | |
dc.description.sponsorship | UK Research & Innovation (UKRI) Science & Technology Facilities Council (STFC) ST/P000711/1 | |
dc.identifier.doi | 10.1393/ncc/i2018-18138-0 | |
dc.identifier.issn | 2037-4909 | |
dc.identifier.issue | 4 | |
dc.identifier.uri | https://doi.org/10.1393/ncc/i2018-18138-0 | |
dc.identifier.uri | https://hdl.handle.net/11452/47571 | |
dc.identifier.volume | 41 | |
dc.identifier.wos | 000459068400010 | |
dc.indexed.wos | WOS.ESCI | |
dc.language.iso | en | |
dc.publisher | Soc Italiana Fisica | |
dc.relation.journal | Nuovo Cimento C-colloquia And Communications In Physics | |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.subject | Exclusion bounds | |
dc.subject | Higgs sectors | |
dc.subject | Tevatron | |
dc.subject | Lep | |
dc.subject | Science & technology | |
dc.subject | Physical sciences | |
dc.subject | Physics, multidisciplinary | |
dc.subject | Physics | |
dc.title | Prospects for sneutrino dark matter in the blssm | |
dc.type | Article | |
dspace.entity.type | Publication | |
relation.isAuthorOfPublication | 0c6ad07c-f6f6-4949-a2f0-e288af6b9411 | |
relation.isAuthorOfPublication.latestForDiscovery | 0c6ad07c-f6f6-4949-a2f0-e288af6b9411 |