Combining the data of annual modulation effect in WIMP direct detection with measurements of WIMP indirect searches
arXiv:hep-ph/9809239 · doi:10.1016/S0927-6505(98)00053-X
Abstract
In previous papers we showed that the data of the DAMA/NaI experiment for WIMP direct detection, which indicate a possible annual modulation effect, are widely compatible with an interpretation in terms of a relic neutralino as the major component of dark matter in the Universe. In the present note we discuss the detectability of the relevant supersymmetric neutralino configurations by two of the most promising methods of indirect search for relic particles: measurement of cosmic-ray antiprotons and measurement of neutrino fluxes from Earth and Sun.
10 pages, ReVTeX, 8 figures (included as PS files)
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- Exploration of Elastic Scattering Rates for Supersymmetric Dark Matter
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- Investigation on light dark matter
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- Enhanced neutrino signals from dark matter annihilation in the Sun via metastable mediators
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- Further investigation of a relic neutralino as a possible origin of an annual-modulation effect in WIMP direct search
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- Can Heavy WIMPs Be Captured by the Earth?
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- Mixed Higgsino Dark Matter from a Large SU(2) Gaugino Mass
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