From classical to quantum Oppenheimer-Snyder model: non-marginal case
arXiv:2303.17924 · doi:10.1103/PhysRevD.107.126006
Abstract
We first present a consistent canonical formulation of the general (non-marginal) Oppenheimer-Snyder model. The switching between comoving and stationary observer is achieved by promoting coordinate transformations between dust proper time and Schwarzschild-Killing time to canonical ones. This leads to a multivalued Hamiltonian which is deparameterizable. We then discuss the quantization of comoving and stationary observers by employing the method of Affine Coherent State Quantization (ACSQ). We thereby demonstrate that under certain conditions the quantum corrected trajectories can replace the classical singularity by a bounce. We then show that both comoving and stationary observers see this bouncing collapse behavior. We finally discuss a switching between these classes of observers at the quantum level.
arXiv comment22 pages, 10 figures, typos corrected, references added
References in corpus (20)
- Dust as a Standard of Space and Time in Canonical Quantum Gravity
- Geometrodynamics of Schwarzschild Black Holes
- Regular coordinate systems for Schwarzschild and other spherical spacetimes
- Classical collapse to black holes and quantum bounces: A review
- Singularity avoidance by collapsing shells in quantum gravity
- Integral quantizations with two basic examples
- Singularity avoidance for collapsing quantum dust in the Lemaitre-Tolman-Bondi model
- Smooth Big Bounce from Affine Quantization
- Bouncing compact objects I: Quantum extension of the Oppenheimer-Snyder collapse
- Singularity avoidance in Bianchi I quantum cosmology
- Towards a quantum Oppenheimer-Snyder model
- Bouncing compact objects. Part II: Effective theory of a pulsating Planck star
- Branched Quantization
- Quantum Oppenheimer-Snyder model
- Phantom singularities and their quantum fate: general relativity and beyond
- Covariant Affine Integral Quantization(s)
- POVM Quantization
- Robustness of the quantum BKL scenario
- Annihilation-to-nothing: DeWitt boundary condition inside a black hole
- Hamiltonian formalism for the Oppenheimer-Snyder model
Cited by in corpus (5)
- Non-Singular Gravitational Collapse through Modified Heisenberg Algebra
- Spin foam amplitude of the black-to-white hole transition
- Quantum theory of the Lemaitre model for gravitational collapse
- Effective Quantum Gravitational Collapse in a Polymer Framework
- Cosmic inflation prevents singularity formation in collapse into a Hayward black hole