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dc.date.accessioned 2022-06-30T14:32:37Z
dc.date.available 2022-06-30T14:32:37Z
dc.date.issued 2021-09-07
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/138638
dc.description.abstract In the LHC searches for gluinos it is usually assumed that they decay predominantly into the lightest neutralino plus jets. In this work we perform a proof-of-concept collider analysis of a novel supersymmetric signal in which gluinos decay mostly into jets and the bino-like neutralino (χ˜ 0 3), which in turn decays into the lightest Higgsino-like neutralino (χ˜ 0 1), considered the dark matter candidate, together with the SM-like Higgs boson (h). This new physics signal then consists of an LHC final state made up by four light jets, four b-jets, and a large amount of missing transverse energy. We identify t¯t, V þ jets (V ¼ W, Z), and t¯t þ X (X ¼ W, Z, γ, h) productions as the most problematic backgrounds, and develop a search strategy for the high luminosity phase of the LHC, reaching signal significances at the evidence level for a luminosity of 1000 fb−1. The prospects for a luminosity of 3000 fb−1 are even more promising, with discovery-level significances. en
dc.language en es
dc.title Novel Higgsino dark matter signal interpretation at the LHC en
dc.type Articulo es
sedici.identifier.other doi:10.1103/physrevd.104.055003 es
sedici.identifier.issn 2470-0010 es
sedici.identifier.issn 2470-0029 es
sedici.creator.person Arganda Carreras, Ernesto es
sedici.creator.person Delgado, Antonio es
sedici.creator.person Morales, Roberto Aníbal es
sedici.creator.person Quirós, Mariano es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 104, no. 5 es


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