7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

A new channel to form near- and sub-solar-mass black holes and naked singularities

9 Jul 2024, 17:40
20m
Sala 17 (Aurum)

Sala 17

Aurum

Largo Gardone Riviera, Pescara, Italy
Invited talk in a parallel session Black hole formation, evolution and the black hole mass gap Black hole formation, evolution and the black hole mass gap

Speaker

Chandrachur Chakraborty (Manipal Centre for Natural Sciences, MAHE, INDIA)

Description

Existence of naked singularities is a topical and fundamental issue of physics. The formation mechanism of such objects, particularly those with near-solar-mass, is not yet clear. Since, recent gravitational wave events have suggested the existence of near-solar-mass collapsed objects which cannot be formed via stellar evolution, here we investigate a likely formation channel, and especially if a near-solar-mass cosmic object can be transmuted into a Kerr naked singularity by capturing
primordial dark matter particles. If the dynamical ejecta is small during the transmutation, the said cosmic object could be transmuted to a Kerr naked singularity. On the other hand, if the dynamical ejecta is large, the same will be transmuted to a sub-solar mass Kerr BH. We show that many white dwarfs could transmute into Kerr naked singularities or a sub-solar mass Kerr BHs (depending on the amount of dynamical ejecta), while neutron stars may not, and mention plausible observational
implications (https://arxiv.org/abs/2401.08462).

Primary author

Chandrachur Chakraborty (Manipal Centre for Natural Sciences, MAHE, INDIA)

Co-author

Prof. Sudip Bhattacharya (Tata Institute of Fundamental Research, Mumbai 400005, India)

Presentation materials

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