Probing Relatively Heavier Right-Handed Selectron at the CEPC, $\rm\bf {FCC_{ee}}$ and ILC
Waqas Ahmed, Imtiaz Khan, Tianjun Li, Shabbar Raza, Wenxing Zhang

TL;DR
This paper investigates the potential to detect relatively heavier right-handed selectrons at future lepton colliders like CEPC, FCC-ee, and ILC, within the MSSM framework, focusing on mono-photon signatures and parameter space constraints.
Contribution
It proposes a novel search strategy for heavier right-handed selectrons at future colliders using mono-photon channels, considering specific MSSM parameter spaces consistent with dark matter and collider bounds.
Findings
Right-handed selectron can be light within certain MSSM parameter spaces.
Future colliders can exclude selectron masses up to 180-210 GeV depending on the scenario.
Mono-photon channel is effective for probing heavier right-handed selectrons.
Abstract
We employ the low energy Minimal Supersymmetric Standard Model (MSSM) to explore the parameter space associated with -pole and Higgs-pole solutions. Such parameter spaces can not only saturate the cold dark matter relic density bound within 5 set by the Planck 2018, but also satisfy the other standard collider mass bounds and B-physics bounds. In particular, we show that the right-handed selectron can be light. Thus, we propose a search for the relatively heavier right-handed selectron at the future lepton colliders with the center-of-mass energy GeV and integrated luminosity 3000 via mono-photon channel: . We show that for the -pole case the right-handed selectron will be excluded up to 180 GeV and 210 GeV respectively at 3 and 2,…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsParticle physics theoretical and experimental studies · Computational Physics and Python Applications · Dark Matter and Cosmic Phenomena
