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Growth of Black Holes in the interior of Rotating Neutron Stars · Around

2013

Growth of Black Holes in the interior of Rotating Neutron Stars

Kouvaris, Chris, Tinyakov, Peter

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Mini-black holes made of dark matter that can potentially form in the interior of neutron stars have been always thought to grow by accreting the matter of the core of the star via a spherical Bondi accretion.

However, neutron stars have sometimes significant angulal velocities that can in principle stall the spherical accretion and potentially change the conclusions derived about the time it takes for black holes to destroy a star.
We study the effect of the star rotation on the growth of such black holes and the evolution of the black hole spin.
Assuming no mechanisms of angular momentum evacuation, we find that even moderate rotation rates can in fact destroy spherical accretion at the early stages of the black hole growth.

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