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Dark matter can be captured by celestial objects and accumulate at their centers, forming a core of dark matter that can collapse to a small black hole, provided that the annihilation rate is small or zero.
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2002
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2013
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K. M. Zurek, Asymmetric Dark Matter: Theories, Signatures, and Constraints
2014
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2014
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2014
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J. Bramante, Dark matter ignition of type Ia supernovae
2015
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2015
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2015
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2015
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J. Bramante and T. Linden, On the r r -Process Enrichment of Dwarf Spheroidal Galaxies
2016
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2016
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2017
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J. Bramante, A. Delgado, and A. Martin, Multiscatter stellar capture of dark matter
2017
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M. Lisanti, Lectures on Dark Matter Physics · 2017
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Fossat, E., Boumier, P., Corbard, T., Provost, J., Salabert, D., Schmider, F. X., Gabriel, A. H., Grec, G., Renaud, C., Robillot, J. M., Roca-Cortés, T., Turck-Chièze, S., Ulrich, R. K., and Lazrek, M., Asymptotic g modes: Evidence for a rapid rotation of the solar core
2017
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2017
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2017
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2018
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C. Kouvaris, P. Tinyakov, and M. H. Tytgat, NonPrimordial Solar Mass Black Holes
2018
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2018
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N. Raj, P. Tanedo, and H.-B. Yu, Neutron stars at the dark matter direct detection frontier
2018
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N. F. Bell, G. Busoni, and S. Robles, Heating up Neutron Stars with Inelastic Dark Matter
2018
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2018
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H. S. Wang, C. H. Lineweaver, and T. R. Ireland, The elemental abundances (with uncertainties) of the most earth-like planet
2018
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2018
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2018
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2018
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2019
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A. J. Deason, A. Fattahi, V. Belokurov, N. W. Evans, R. J. J. Grand, F. Marinacci, and R. Pakmor, The local high-velocity tail and the galactic escape speed
2019
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2019
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2019
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