activity
20242026
collaborators

13 papers

astro-ph.HE2026

Transmutation Timescales for Dark Matter Induced Collapse of Compact Stars into Black Holes

H. A. Adarsha, Chandrachur Chakraborty, Sudip Bhattacharyya

Ultra-heavy asymmetric dark matter (DM) particles captured by compact stars can thermalize, self-gravitate, and collapse to form an endoparasitic black hole (EBH), whose subsequent…

astro-ph.HE2026

Tilted thin accretion disks in the full Kerr spacetime and their implications

K. S. Sruthy, Chandrachur Chakraborty, Sudip Bhattacharyya

We derive a steady-state warped-disk equation in the full Kerr spacetime to study the tilt dynamics of a thin, viscous accretion disk around a spinning collapsed object. The formul…

astro-ph.HE2026

A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588

Vaidehi Poojyam, Vikas Mistry, Yash Bhargava +2

Neutron star (NS) low-mass X-ray binary (LMXB) systems depict a variety of X-ray spectral and timing features, which can be useful to probe the accretion-ejection mechanism in the…

astro-ph.HE2026

Degeneracy in Accretion Disk Spectra from Naked Singularities and Kerr Black Holes: Application to the AGN MCG-06-30-15

Vishva Patel, Sayantan Bhattacharya, Sudip Bhattacharyya +1

Theoretical studies suggest that gravitational collapse can form either a black hole or a visible (naked) singularity. Identifying observational signatures that distinguish these t…

astro-ph.HE2026

Magnetically arrested transmutation of a compact star

H. A. Adarsha, Chandrachur Chakraborty, Sudip Bhattacharyya

We introduce a novel mechanism -- Magnetically Arrested Transmutation (MAT) -- which could be a viable model to account for the observed over-representation of magnetic white dwarf…

gr-qc2026

Tidal disruption of a neutron star near naked singularity

Ashok B. Joshi, Pankaj S. Joshi, Sudip Bhattacharyya

We investigate the tidal disruption of a neutron star (NS) near a black hole (BH), and for the first time, to the best of our knowledge, near a naked singularity (NaS). For a BH wi…