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- W2016400599 abstract "We study the capture of dark matter particles by neutron stars in close binary systems. By performing a direct numerical simulation, we find that there is a sizable amplification of the rate of dark matter capture by each of the companions. In the case of the binary pulsar PSR $mathrm{J}1906+0746$ with the orbital period of 4 hours the amplification factor is $ensuremath{simeq}3.5$. This amplification can be attributed to the energy loss by dark matter particles resulting from their gravitational scattering off moving companions." @default.
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- W2016400599 date "2012-08-08" @default.
- W2016400599 modified "2023-10-18" @default.
- W2016400599 title "Enhancement of Dark Matter Capture by Neutron Stars in Binary Systems" @default.
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- W2016400599 doi "https://doi.org/10.1103/physrevlett.109.061301" @default.
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