Light neutralinos with large scattering cross sections in the minimal supersymmetric standard model
- Creators
- Kuflik, Eric
- Pierce, Aaron
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Zurek, Kathryn M.
Abstract
Motivated by recent data from CoGeNT and the DAMA annual modulation signal, we discuss collider constraints on the minimal supersymmetric standard model neutralino dark matter with mass in the 5–15 GeV range. The lightest superpartner (LSP) would be a bino with a small Higgsino admixture. Maximization of the dark matter nucleon scattering cross section for such a weakly interacting massive particle requires a light Higgs boson with tan β enhanced couplings. Limits on the invisible width of the Z boson, combined with the rare decays B^± → τν, and the ratio B → Dτν/B → Dℓν, constrain cross sections to be below σ_n ≲ 5 × 10^(−42) cm^2. This indicates a higher local dark matter density than is usually assumed by a factor of roughly 6 necessary to explain the CoGeNT excess. This scenario also requires a light charged Higgs boson, which can give substantial contributions to rare decays such as b → sγ and t → bH^+. We also discuss the impact of Tevatron searches for Higgs bosons at large tan β.
Additional Information
© 2010 American Physical Society. (Received 16 March 2010; published 28 June 2010) We thank Tim Cohen and Dan Phalen for discussions. A. P. was supported in part by NSF Career Grant No. NSF-PHY-0743315 and in part by DOE Grant No. DE-FG02-95ER40899. E. K. acknowledges support from NSF Grant No. PHY/0917807 and from DOE Grant No. DE-FG02-95ER40899.Attached Files
Published - PhysRevD.81.111701.pdf
Accepted Version - 1003.0682.pdf
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Additional details
- Eprint ID
- 96372
- Resolver ID
- CaltechAUTHORS:20190613-110921243
- NSF
- PHY-0743315
- Department of Energy (DOE)
- DE-FG02-95ER40899
- NSF
- PHY-0917807
- Department of Energy (DOE)
- DE-FG02-95ER40899
- Created
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2019-06-13Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field