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 $\mathrm{tan}\ensuremath{\beta}$ enhanced couplings. Limits on the invisible width of the $Z$ boson, combined with the rare decays ${B}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\rightarrow}\ensuremath{\tau}\ensuremath{\nu}$, and the ratio $B\ensuremath{\rightarrow}D\ensuremath{\tau}\ensuremath{\nu}/B\ensuremath{\rightarrow}D\ensuremath{\ell}\ensuremath{\nu}$, constrain cross sections to be below ${\ensuremath{\sigma}}_{n}\ensuremath{\lesssim}5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}42}\text{ }\text{ }{\mathrm{cm}}^{2}$. 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 $b\ensuremath{\rightarrow}s\ensuremath{\gamma}$ and $t\ensuremath{\rightarrow}b{H}^{+}$. We also discuss the impact of Tevatron searches for Higgs bosons at large $\mathrm{tan}\ensuremath{\beta}$.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.