Low Mass Naked Singularities from Dark Core Collapse
Chandrachur Chakraborty (MCNS, India), Sudip Bhattacharyya (TIFR,, India), Pankaj S. Joshi (Ahmedabad U., India)

TL;DR
This paper explores how dark matter-induced core collapse in neutron stars could produce either black holes or naked singularities, with implications for gravitational wave sources and pulsar observations.
Contribution
It introduces the possibility of naked singularity formation from dark matter core collapse, challenging the exclusive focus on black holes in such processes.
Findings
Dark matter core collapse can lead to naked singularities instead of black holes.
Naked singularities can transmute neutron stars into near-solar mass objects.
Missing pulsars near the Galactic center may indicate the presence of naked singularities.
Abstract
Near-solar mass black holes (BHs) could have been involved in the two recent gravitational wave events, GW190425 and GW190814. Since such a low mass BH cannot be formed via stellar evolution, a model has been proposed based on the core collapse of a neutron star initiated by a certain number of dark matter (DM) particles. In this process, the accumulated DM particles collapse to form a tiny BH inside the neutron star, and the entire neutron star is transmuted into a BH after a certain time due to the accretion of matter by the endoparasitic BH from its host. Here, we argue that, depending on the initial conditions, a dark core collapse could give rise to either a BH or a naked singularity. For example, if the accumulated cloud of DM particles in the core of a neutron star can be modeled as an anisotropic fluid and it fulfils the criterion for collapse, an endoparasitic naked singularity…
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