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Results and prospects of dark matter searches with ANTARES · Around

2014

Results and prospects of dark matter searches with ANTARES

Zornoza, J. D., Lambard, G.

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Understand

Dark matter is one of the most important scientific goals for neutrino telescopes.

These instruments have particular advantages with respect to other experimental approaches.
Compared to direct searches, the sensitivity of neutrino telescopes to probe the spin-dependent cross section of WIMP-proton is unsurpassed.
On the other hand, neutrino telescopes can look for dark matter in the Sun, so a potential signal would be a strong indication of dark matter, contrary to the case of other indirect searches like gammas or cosmic rays, where more conventional astrophysical interpretations are very hard to rule out.

Built on

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P. Gondolo et al., “DarkSUSY: Computing Supersymmetric Dark Matter Properties Numerically”, J. Cosm. and Astropart. Phys., JCAP07, 008 (2004)
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Similar

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2008
Cited alongside, same era.
J. Ellis et al., “Neutrino Fluxes from CMSSM LSP Annihilations in the Sun”, Phys. Rev. D 81
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M. Ageron et al
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2011
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Then

T. Tanaka et al., Super-Kamiokande Collaboration, “An Indirect Search for WIMPs in the Sun using 3109.6 days of upward-going muons in Super-Kamiokande”, Astrophys. J. 742
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M. Felizardo et al., SIMPLE Collaboration, “Final Analysis and Results of the Phase II SIMPLE Dark Matter Search”, Phys. Rev. Lett. 108
2012
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E. Behnke et al., COUPP Collaboration, “First dark matter search results from a 4-kg CF 3 I bubble chamber operated in a deep underground site”, Phys. Rev. D 86
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Original
2013
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