Beyond Hawking evaporation of black holes formed by dark matter in compact stars
arXiv:2410.22702 · doi:10.1103/PhysRevD.111.L041306
Abstract
The memory burden effect is an explicit resolution to the information paradox by which an evaporating black hole acquires quantum hair, which then suppresses its rate of mass loss with respect to the semi-classical Hawking rate. We show that this has significant implications for particle dark matter that captures in neutron stars and forms black holes that go on to consume the host star. In particular, we show that constraints on the nucleon scattering cross section and mass of spin-0 and spin-1/2 dark matter would be extended by several orders of magnitude.
4 pages revtex + references, 1 figure; v2 matches PRD
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- Impact of memory-burdened primordial black holes on high-scale leptogenesis
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- Stronger Constraints on Primordial Black Holes as Dark Matter Derived from the Thermal Evolution of the Intergalactic Medium over the Last Twelve Billion Years
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- From Capture to Collapse: Revisiting Black Hole formation by Fermionic Asymmetric Dark Matter in Neutron Stars
- Memory burden effect of regular primordial black holes