Abstract
We perform an indirect search for weakly interacting massive particles (WIMPs) using the MACRO detector to look for neutrino-induced upward-going muons resulting from the annihilation of WIMPs trapped in the Sun and Earth. The search is conducted in various angular cones centered on the Sun and Earth to accommodate a range of WIMP masses. No significant excess over the background from atmospheric neutrinos is seen. We set experimental flux limits on the upward-going muon fluxes from the Sun and the Earth. These limits are used to constrain neutralino particle parameters from supersymmetric theory, including those suggested by recent results from DAMA-NaI.
Lingua originale | Inglese |
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Rivista | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volume | 60 |
Numero di pubblicazione | 8 |
DOI | |
Stato di pubblicazione | Pubblicato - 1999 |
Pubblicato esternamente | Sì |