Clustered dark matter may enable small seed black holes to grow to over 10^7 solar masses by redshift 10 in dense nuclear star clusters, with special behavior for ultralight dark matter due to its de Broglie wavelength.
Phys Rev D 96(8):083014
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This review summarizes tidal Love numbers and dissipation effects for black holes, neutron stars, and exotic objects, noting vanishing static bosonic Love numbers for black holes in GR but nonzero values for fermions and exotic objects, with implications for gravitational-wave astronomy.
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Dark Matter and the Early Formation of Supermassive Black Holes
Clustered dark matter may enable small seed black holes to grow to over 10^7 solar masses by redshift 10 in dense nuclear star clusters, with special behavior for ultralight dark matter due to its de Broglie wavelength.
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Tidal Response of Compact Objects
This review summarizes tidal Love numbers and dissipation effects for black holes, neutron stars, and exotic objects, noting vanishing static bosonic Love numbers for black holes in GR but nonzero values for fermions and exotic objects, with implications for gravitational-wave astronomy.