Testing the gaugino AMSB model at the Tevatron via slepton pair production
Howard Baer, Senarath de Alwis, Kevin Givens, Shibi Rajagopalan and, Warintorn Sreethawong

TL;DR
This paper investigates the potential for the Tevatron collider to detect gaugino AMSB models through slepton pair production, highlighting observable signals like leptons and chargino tracks, and estimating the experimental reach.
Contribution
It provides the first detailed calculation of slepton pair production signals in gaugino AMSB models at the Tevatron, including chargino tracks and their detectability.
Findings
Tevatron can probe gravitino masses up to ~55 TeV.
Gluino mass reach exceeds 1100 GeV.
Observable signals include leptons and highly ionizing tracks.
Abstract
Gaugino AMSB models-- wherein scalar and trilinear soft SUSY breaking terms are suppressed at the GUT scale while gaugino masses adopt the AMSB form-- yield a characteristic SUSY particle mass spectrum with light sleptons along with a nearly degenerate wino-like lightest neutralino and quasi-stable chargino. The left- sleptons and sneutrinos can be pair produced at sufficiently high rates to yield observable signals at the Fermilab Tevatron. We calculate the rate for isolated single and dilepton plus missing energy signals, along with the presence of one or two highly ionizing chargino tracks. We find that Tevatron experiments should be able to probe gravitino masses into the ~55 TeV range for inoAMSB models, which corresponds to a reach in gluino mass of over 1100 GeV.
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