Free Meson Seminars

Neutron Star Quantum Death by Small Black Holes

by Prof. Stefano Profumo (University of California, Santa Cruz, USA)

Friday, July 16, 2021 from to (Asia/Kolkata)
at Zoom
Description Please contact rishi(at)theory(dot)tifr(dot)res(dot)in for the zoom meeting id and the password for this seminar.

Neutron stars can be destroyed by black holes at their center accreting material and eventually swallowing the entire star. I will argue that the accretion model adopted in the literature, based on Bondi accretion or variations thereof, is inadequate for "small" black holes - black holes whose Schwarzschild radius is comparable to, or smaller than, the neutron's de Broglie wavelength. In this case, quantum mechanical aspects of the accretion process cannot be neglected, and give rise to a completely different accretion rate. I will show that for the case of black holes seeded by the collapse of bosonic dark matter, this is the case for electroweak-scale dark matter particles. In the case of fermionic dark matter, typically the black holes that would form at the center of a neutron star are more massive, unless the dark matter particle mass is very large, larger than about 1010 GeV. I calculate the lifetime of neutron stars harboring a "small" black hole, and find that black holes lighter than ∼1011∼1012 kg quickly evaporate, leaving no trace. More massive black holes destroy neutron stars via quantum accretion on time-scales much shorter than the age of observed neutron stars.

https://www.youtube.com/watch?v=9yGxwdKa18A
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