Extending the weak cosmic censorship conjecture to the charged Buchdahl star by employing the gedanken experiments
arXiv:2205.01350 · doi:10.1088/1475-7516/2023/06/010
Abstract
In this paper, we wish to investigate the weak cosmic censorship conjecture (WCCC) for the non black hole object, Buchdahl star and test its validity. It turns out that the extremal limit for the star is over-extremal for black hole, ; i.e., it could have . By carrying out both linear and non-linear perturbations, we establish the same result for the Buchdahl star as well. That is, as for black hole it could be overcharged at the linear perturbation while the result is overturned when the non-linear perturbations are included. Thus WCCC is always obeyed by the Buchdahl star.
17 pages, no figures. Updated to match with the published version
References in corpus (16)
- Gedanken Experiments to Destroy a Black Hole II: Kerr-Newman Black Holes Cannot be Over-Charged or Over-Spun
- Destroying a near-extremal Kerr-Newman black hole
- Overspinning a Kerr black hole: the effect of self-force
- Weak cosmic censorship conjecture for the novel charged Einstein-Gauss-Bonnet black hole with test scalar field and particle
- Gravitational perturbation of the BTZ black hole induced by test particles and weak cosmic censorship in AdS spacetime
- Overcharging higher-dimensional black holes with point particles
- Destroying a near-extremal Kerr black hole with a charged particle: Can a test magnetic field serve as a cosmic censor?
- Can test fields destroy the event horizon in the Kerr-Taub-NUT spacetime?
- Weak cosmic censorship conjecture for Kerr-Taub-NUT black hole with test scalar field and particle
- Compactness bounds in General Relativity
- Weak cosmic censorship conjecture in Einstein-Born-Infeld black holes
- On overspinning of black holes in higher dimensions
- Testing the weak cosmic censorship conjecture for a Reissner-Nordström-de Sitter black hole surrounded by perfect fluid dark matter
- Maximum Force for Black Holes and Buchdahl Stars
- Upper bound on the gravitational masses of stable spatially regular charged compact objects
- Universality of the Buchdahl sphere