Abstract

Neutrino telescopes have a wide scientific scope. One of their main goals is the detection of dark matter, for which they have specific advantages. Neutrino telescopes offer the possibility of looking at several kinds of sources, not all of them available to other indirect searches. In this work we provide an overview of the results obtained by the ANTARES neutrino telescope, which has been taking data for almost ten years. One of the most interesting ones is the Sun, since a detection of high energy neutrinos from it would be a very clean indication of dark matter, given that no significant astrophysical backgrounds are expected, contrary to other indirect searches. Moreover, the limits from neutrino telescopes for spin-dependent cross section are the most restrictive ones. Another interesting source is the Galactic Centre, for which ANTARES has a better visibility than IceCube, due to its geographical location. This search gives limits on the annihilation cross section. Other dark matter searches carried out in ANTARES include the Earth and dwarf galaxies.

Highlights

  • Neutrino telescopes have a wide scientific scope

  • The results presented in this work include searches for neutrino excess from several astrophysical sources

  • The limits from neutrino telescopes for spin-dependent cross section are the most restrictive ones. Another interesting source is the Galactic Centre, for which ANTARES has a better visibility than IceCube, due to its geographical location

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Summary

The ANTARES detector

Neutrino astronomy has specific advantages with respect to other ways to study the universe The ANTARES [1] neutrino telescope was completed in 2008. Only muons are used, since they offer the best angular resolution

Artistic view of ANTARES
Dark matter detection
Dwarf galaxies
Newest results!
Other sources
Conclusions
Full Text
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