Can we distinguish black holes from naked singularities by the images of their accretion disks?
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Publication:5067155
DOI10.1088/1475-7516/2019/10/064OpenAlexW2974043736MaRDI QIDQ5067155
Rajibul Shaikh, Pankaj S. Joshi
Publication date: 1 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1909.10322
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Cites Work
- Self-gravitating fluid systems and galactic dark matter
- A novel gravitational lensing feature by wormholes
- Observational distinction between black holes and naked singularities: the role of the redshift function
- Appearance of Keplerian discs orbiting Kerr superspinars
- Equilibrium configurations from gravitational collapse
- Counter-rotating Keplerian discs around Kerr superspinars
- The final fate of spherical inhomogeneous dust collapse
- RECENT DEVELOPMENTS IN GRAVITATIONAL COLLAPSE AND SPACETIME SINGULARITIES
- Shadow images of Kerr-like wormholes
- Distinguishing black holes from naked singularities through their accretion disc properties
- Gravitational Collapse and Spacetime Singularities
- The final fate of spherical inhomogeneous dust collapse: II. Initial data and causal structure of the singularity
- Circular orbits in Kerr-Taub-NUT spacetime and their implications for accreting black holes and naked singularities
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