Novel Higgsino dark matter signal interpretation at the LHC
Ernesto Arganda (IFLP, CONICET—Dpto. de Física, Universidad Nacional de La Plata, C.C. 67, 1900 La Plata, Argentina, Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13-15, Campus de Cantoblanco, 28049 Madrid, Spain); Antonio Delgado (Department of Physics, University of Notre Dame, 225 Nieuwland Hall Notre Dame, Indiana 46556, USA); Roberto A. Morales (Instituto de Física Teórica UAM/CSIC, C/ Nicolás Cabrera 13-15, Campus de Cantoblanco, 28049 Madrid, Spain); Mariano Quirós (Institut de Física d’Altes Energies (IFAE) and BIST, Campus UAB 08193, Bellaterra, Barcelona, Spain)
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 (), which in turn decays into the lightest Higgsino-like neutralino (), considered the dark matter candidate, together with the SM-like Higgs boson (). This new physics signal then consists of an LHC final state made up by four light jets, four -jets, and a large amount of missing transverse energy. We identify , (, ), and (, , , ) 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 . The prospects for a luminosity of are even more promising, with discovery-level significances.