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• W3181715181 abstract "We consider a scenario where light bino is the next-to-lightest supersymmetric particle (NLSP) and gravitino/axino is the lightest superysmmetric particle (LSP). For a bino mass less than or around hundred GeV, it can be pair produced at the future lepton colliders through $tensuremath{-}$channel slepton exchange, subsequently decaying into a gravitino/axino plus a photon. We study the prospects to look for such binos at the future colliders and find that a bino mass around 100 GeV can be probed at the $2ensuremath{sigma}$ ($5ensuremath{sigma}$) level for a slepton below 2 TeV (1.5 TeV) with a luminosity $5.6text{ }text{ }{mathrm{ab}}^{ensuremath{-}1}$. For a bino mass around 10 GeV, a slepton mass less than 4.5 TeV (3.5 TeV) can be probed at the $2ensuremath{sigma}$ ($5ensuremath{sigma}$) level, which is much beyond the reach of the LHC for direct slepton searches." @default.
• W3181715181 created "2021-07-19" @default.
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• W3181715181 date "2021-07-07" @default.
• W3181715181 modified "2023-10-17" @default.
• W3181715181 title "Probing a bino NLSP at lepton colliders" @default.
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• W3181715181 doi "https://doi.org/10.1103/physrevd.104.015009" @default.
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