Beyond Hawking evaporation of black holes formed by dark matter in compact stars

Fuente: arXiv
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Auteurs principaux: Basumatary, Ujjwal, Raj, Nirmal, Ray, Anupam
Format: Preprint
Publié: 2024
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author Basumatary, Ujjwal
Raj, Nirmal
Ray, Anupam
author_facet Basumatary, Ujjwal
Raj, Nirmal
Ray, Anupam
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2410_22702
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Beyond Hawking evaporation of black holes formed by dark matter in compact stars
Basumatary, Ujjwal
Raj, Nirmal
Ray, Anupam
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
High Energy Physics - Theory
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.
title Beyond Hawking evaporation of black holes formed by dark matter in compact stars
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
High Energy Physics - Experiment
High Energy Physics - Theory
url https://arxiv.org/abs/2410.22702