Light $\stop\to\wino b$ models are not ruled out by the Tevatron top experiments
| dc.creator | Sender, John | |
| dc.date | 1996-02-20 | |
| dc.date.accessioned | 2026-07-07T03:58:54Z | |
| dc.date.available | 2026-07-07T03:58:54Z | |
| dc.description | SUSY events in which a light stop decays to a chargino may manage to pass the cuts designed for top counting experiments at the Tevatron with no significant diminution of signal. Events in which a top decays via stop are detected with fair efficiency compared to SM top events when $\stop\into b\wino$. More importantly, direct pair production of light stops contributes significantly to the cut samples. Many SUSY models with stops lighter than 100 GeV are viable even for $Γ(t\into\stop) \approx Γ(t\into bW)$. | |
| dc.description | 7 pages, 3 postscript figures, uses epsf.sty | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9602354 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9602354 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/46003 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Light $\stop\to\wino b$ models are not ruled out by the Tevatron top experiments | |
| dc.type | text |