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Dark matter could be captured in the Sun and self-annihilate, giving rise to an observable neutrino flux.
- Indirect searches for dark matter looking for this signal with neutrino telescopes have resulted in tight constraints on the interaction cross-section of dark matter with ordinary matter.
- We investigate how robust limits are against astro-physical uncertainties.
- We study the effect of the velocity distribution of dark matter in our Galaxy on capture rates in the Sun.
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