Light Higgsino Detection at LEP1.5
| dc.creator | Ambrosanio, S. | |
| dc.creator | Carena, M. | |
| dc.creator | Mele, B. | |
| dc.creator | Wagner, C. E. M. | |
| dc.date | 1995-11-07 | |
| dc.date | 1996-10-17 | |
| dc.date.accessioned | 2026-07-07T10:58:13Z | |
| dc.date.available | 2026-07-07T10:58:13Z | |
| dc.description | Within the minimal supersymmetric extension of the Standard Model, the best fit to the most recent precision-measurement data requires charginos and neutralinos, with dominant Higgsino components and with masses within the reach of LEP1.5 ($\sqrt{s}=140$ GeV). In this work, we present a detailed analysis of the neutralino and chargino production processes for the favoured region of parameter space, that is low values of $|μ|$ and either low or large values of $\tanβ$. We find that chargino and neutralino searches can cover the Higgsino region in the ($μ,M_2$) plane for values of $M_2 \simlt 1$ TeV, at the next phases of the LEP collider. We also show that, due mainly to phase-space constraints, the lightest neutralinos should be more easily detectable than charginos in most of the parameter space preferred by precision-measurement data. | |
| dc.description | 16 pages, 8 Figures, LateX. Figures now include initial state radiation effects on the cross sections. | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9511259 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9511259 | |
| dc.identifier | Phys.Lett.B373:107-116,1996 | |
| dc.identifier | doi:10.1016/0370-2693(96)00129-3 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/187019 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Light Higgsino Detection at LEP1.5 | |
| dc.type | text |