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DOE OSTI · 1797735

Dark matter detection, Standard Model parameters and Intermediate Scale Supersymmetry

Dunsky, David·Hall, Lawrence J.·Harigaya, Keisuke
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Abstract

The vanishing of the Higgs quartic coupling at a high energy scale may be explained by Intermediate Scale Supersymmetry, where supersymmetry breaks at (10 9 -10 12 ) GeV. The possible range of supersymmetry breaking scales can be narrowed down by precise measurements of the top quark mass and the strong coupling constant. On the other hand, nuclear recoil experiments can probe Higgsino or sneutrino dark matter up to a mass of 1012 GeV. We derive the correlation between the dark matter mass and precision measurements of standard model parameters, including supersymmetric threshold corrections. The dark matter mass is bounded from above as a function of the top quark mass and the strong coupling constant. The top quark mass and the strong coupling constant are bounded from above and below respectively for a given dark matter mass. We also discuss how the observed dark matter abundance can be explained by freeze-out or freeze-in during a matter-dominated era after inflation, with the inflaton condensate being dissipated by thermal effects.

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72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDSCosmology of Theories beyond the SMHiggs PhysicsQuark Masses and SM ParametersSupersymmetric Standard Model

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Dunsky, David, Hall, Lawrence J., Harigaya, Keisuke. 2021-04-07. Dark matter detection, Standard Model parameters and Intermediate Scale Supersymmetry. https://doi.org/10.1007/jhep04(2021)052

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