Comment (2) on "Quantum Transfiguration of Kruskal Black Holes"
arXiv:1906.04650
Abstract
An explicit calculation shows that the model constructed in arXiv:1806.00648 violates general covariance. It is therefore unphysical and does not determine properties of space-time or black holes.
2 pages
Cited by in corpus (12)
- Critical evaluation of common claims in loop quantum cosmology
- (b,v)-type variables for black to white hole transitions in effective loop quantum gravity
- Properties of the spherically symmetric polymer black holes
- Bouncing compact objects. Part II: Effective theory of a pulsating Planck star
- Annihilation-to-nothing: a quantum gravitational boundary condition for the Schwarzschild black hole
- Quantum dynamics of the black hole interior in LQC
- Massless Dirac Perturbations in a Consistent Model of Loop Quantum Gravity Black Hole: Quasinormal Modes and Particle Emission Rates
- Annihilation-to-nothing: DeWitt boundary condition inside a black hole
- Quantum Corrected Polymer Black Hole Thermodynamics: Mass Relations and Logarithmic Entropy Correction
- Quantum gravitational wave function for the interior of a black hole and the generalized uncertainty principle
- Generic features of a polymer quantum black hole
- Black hole or Fuzz ball or a Loop quantum star ? Assessing the fate of a massive collapsing star