Suppressing the Scattering of WIMP DM with Nucleons in Supersymmetric Theories
Junjie Cao, Lei Meng, Yuanfang Yue, Haijing Zhou, Pengxuan Zhu

TL;DR
This paper explores how the inverse seesaw extension of the NMSSM allows sneutrino dark matter to evade scattering constraints and satisfy relic density and collider bounds, highlighting its viability as a weakly interacting dark matter candidate.
Contribution
It demonstrates that the inverse seesaw extension broadens the parameter space where sneutrino dark matter is consistent with experimental constraints in supersymmetric models.
Findings
Inverse seesaw extension allows broader viable parameter space.
Sneutrino dark matter can satisfy relic density and scattering constraints.
Supersymmetric models with inverse seesaw are promising dark matter candidates.
Abstract
The continuously improving sensitivity of dark matter direct detection experiments has limited the interaction between dark matter and nucleons being increasingly feeble, while the dark matter relic density favors it to take part in weak interactions. After taking into account the constraints from the Large Hadron Collider (LHC) search for Higgs bosons and sparticles, it is becoming difficult for the neutralino dark matter in the Minimal Supersymmetric Standard Model and the Next-to-Minimal Supersymmetric Standard Model to possess these two seemingly paradoxical features in their most natural parameter space for electroweak symmetry breaking due to the limited theoretical structure. In contrast, the seesaw extension of the Next-to-Minimal Supersymmetric Standard Model, which was initially proposed to solve the neutrino mass problem, enables the lightest sneutrino to act as a viable dark…
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