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We studied the rate at which stars capture dark matter (DM) particles, considering different assumptions regarding the DM characteristics and in particular investigating how the stellar physics influences the capture rate.
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In the specific case of the present Sun, these results are confirmed by preliminary results presented by J.Edsjö at the workshop Dark Matter All Around, Paris, December 2010, for J. Edsjö, C. Savage, P. Scott, and A. Serenelli (work in progress)
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