Theoretical predictions for the direct detection of neutralino dark matter in the NMSSM

We analyse the direct detection of neutralino dark matter in the framework of the Next-to-Minimal Supersymmetric Standard Model. After performing a detailed analysis of the parameter space, taking into account all the available constraints from LEPII, we compute the neutralino-nucleon cross section, and compare the results with the sensitivity of detectors. We find that sizable values for the detection cross section, within the reach of dark matter detectors, are attainable in this framework. For example, neutralino-proton cross sections compatible with the sensitivity of present experiments can be obtained due to the exchange of very light Higgses with m_{h_1^0}\lsim 70 GeV. Such Higgses have a significant singlet composition, thus escaping detection and being in agreement with accelerator data. The lightest neutralino in these cases exhibits a large singlino-Higgsino composition, and a mass in the range 50\lsim m_{\tilde\chi_1^0}\lsim 100 GeV.

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Final version to appear in JHEP. References added. LaTeX, 53 pages, 23 figures Report-no: DESY 04-129, IFIC/04-44, FTUAM 04/17, IFT-UAM/CSIC-04-42

12.60.Jv
95.35.+d
dark matter
supersymmetry
neutralino: search for
neutralino nucleus: elastic scattering
cross section: mass
Higgs particle: exchange
Higgs particle: mass
potential: Higgs

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