Indirect detection of dark matter in km-size neutrino telescopes
- 27 October 1998
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 58 (10) , 103519
- https://doi.org/10.1103/physrevd.58.103519
Abstract
Neutrino telescopes of kilometer size are currently being planned. They will be two or three orders of magnitude bigger than presently operating detectors, but they will have a much higher muon energy threshold. We discuss the trade-off between area and energy threshold for indirect detection of neutralino dark matter captured in the Sun and in the Earth and annihilating into high energy neutrinos. We also study the effect of a higher threshold on the complementarity of different searches for supersymmetric dark matter.All Related Versions
This publication has 31 references indexed in Scilit:
- Supersymmetric dark matterPublished by Elsevier ,1999
- Neutralino relic density including coannihilationsPhysical Review D, 1997
- Astrophysical-neutrino detection with angular and energy resolutionAstroparticle Physics, 1997
- Indirect neutralino detection rates in neutrino telescopesPhysical Review D, 1997
- Searching for relic neutralinos using neutrino telescopesAstroparticle Physics, 1996
- Limits on cold-dark-matter candidates from deep underground detectorsPhysical Review D, 1986
- Solar System constraints and signatures for dark-matter candidatesPhysical Review D, 1986
- Can scalar neutrinos or massive Dirac neutrinos be the missing mass?Physics Letters B, 1986
- Capture by the sun of a galactic population of weakly interacting, massive particlesThe Astrophysical Journal, 1985
- The photino, the sun, and high-energy neutrinosPhysical Review Letters, 1985