dc.date.accessioned | 2015-03-12T15:05:20Z | |
dc.date.available | 2015-03-12T15:05:20Z | |
dc.date.created | 2014-09-24T11:53:50Z | |
dc.date.issued | 2014 | |
dc.identifier.citation | Bomark, Nils-Erik Kvellestad, Anders Lola, Smaragda Osland, Per Raklev, Are . Long lived charginos in Natural SUSY?. Journal of High Energy Physics (JHEP). 2014, 2014(5:7) | |
dc.identifier.uri | http://hdl.handle.net/10852/43129 | |
dc.description.abstract | Supersymmetric models with a small chargino-neutralino mass difference, and as a result metastable charginos, have been a popular topic of investigation in collider phenomenology. The possibility of a chargino lighter than the lightest neutralino has also been raised. Recently, the absence of any supersymmetric signal in the 8 TeV LHC data has led to significant interest in the so-called Natural SUSY models with light higgsinos. These models also have a naturally small chargino-neutralino mass difference. However, we show here that when relevant indirect constraints from results at the LHC and elsewhere are applied, this possibility is heavily constrained within the Minimal Supersymmetric Standard Model (MSSM): massive metastable higgsinos are not a signature of Natural SUSY. | en_US |
dc.language | EN | |
dc.language.iso | en | en_US |
dc.publisher | Institute of Physics Publishing (IOPP) | |
dc.relation.ispartof | Anders Kvellestad (2015) Chasing SUSY Through Parameter Space. Doctoral thesis. http://urn.nb.no/URN:NBN:no-51621 | |
dc.relation.uri | http://urn.nb.no/URN:NBN:no-51621 | |
dc.rights | Attribution 4.0 International | |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
dc.title | Long lived charginos in Natural SUSY? | en_US |
dc.type | Journal article | en_US |
dc.creator.author | Bomark, Nils-Erik | |
dc.creator.author | Kvellestad, Anders | |
dc.creator.author | Lola, Smaragda | |
dc.creator.author | Osland, Per | |
dc.creator.author | Raklev, Are | |
cristin.unitcode | 185,15,4,0 | |
cristin.unitname | Fysisk institutt | |
cristin.ispublished | true | |
cristin.fulltext | original | |
cristin.qualitycode | 2 | |
dc.identifier.cristin | 1157516 | |
dc.identifier.bibliographiccitation | info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Journal of High Energy Physics (JHEP)&rft.volume=2014&rft.spage=&rft.date=2014 | |
dc.identifier.jtitle | Journal of High Energy Physics (JHEP) | |
dc.identifier.volume | 2014 | |
dc.identifier.issue | 5 | |
dc.identifier.doi | http://dx.doi.org/10.1007/JHEP05(2014)007 | |
dc.identifier.urn | URN:NBN:no-47503 | |
dc.subject.nvi | VDP::Kjerne- og elementærpartikkelfysikk: 431 | |
dc.type.document | Tidsskriftartikkel | en_US |
dc.type.peerreviewed | Peer reviewed | |
dc.source.issn | 1029-8479 | |
dc.identifier.fulltext | Fulltext https://www.duo.uio.no/bitstream/handle/10852/43129/1/art%25253A10.1007%25252FJHEP05%2525282014%252529007.pdf | |
dc.type.version | PublishedVersion | |
cristin.articleid | 7 | |