Quantum Effective Dynamics of Papapetrou Spacetime
arXiv:2506.08821 · doi:10.1140/epjc/s10052-025-14606-y
Abstract
In this paper, we investigate the quantum effective dynamics of Papapetrou spacetime by using methods from loop quantum gravity. The Papapetrou spacetime is an extension of the Schwarzschild spacetime with an extra coupled anti-scalar field. By solving the equations of motion generated by the Hamiltonian constraint for Papapetrou spacetime, we can construct the quantum effective metric. The resulting effective metric for the quantum-corrected Papapetrou spacetime demonstrates the quantum effects will give rise to a new wormhole throat, while the classical wormhole throat disappear in the case of extremely small mass.
References in corpus (17)
- Quantum geometry and the Schwarzschild singularity
- Quantum Transfiguration of Kruskal Black Holes
- Quantum Extension of the Kruskal Space-time
- Quantum Oppenheimer-Snyder and Swiss Cheese models
- Effective loop quantum gravity framework for vacuum spherically symmetric space-times
- An effective model for the quantum Schwarzschild black hole
- The exponential metric represents a traversable wormhole
- Black Holes and Covariance in Effective Quantum Gravity
- Simpler than vacuum: Antiscalar alternatives to black holes
- Polymer quantization of the Einstein-Rosen wormhole throat
- Lorentzian wormhole in the framework of loop quantum cosmology
- Nonexistence of quantum black and white hole horizons in an improved dynamic approach
- Quantum geometry and effective dynamics of Janis-Newman-Winicour singularities
- Quantum dynamics of the Einstein-Rosen wormhole throat
- Traversable Wormholes Sourced by Dark Matter in Loop Quantum Cosmology
- Anisotropic Structures and Wormholes with Loop Quantum Gravity Holonomy Corrections
- Non-singular naked solutions in quantum spacetime