Information loss, made worse by quantum gravity?
arXiv:1409.3157 · doi:10.3389/fphy.2015.00033
Abstract
Quantum gravity is often expected to solve both the singularity problem and the information-loss problem of black holes. This article presents an example from loop quantum gravity in which the singularity problem is solved in such a way that the information-loss problem is made worse. Quantum effects in this scenario, in contrast to previous non-singular models, do not eliminate the event horizon and introduce a new Cauchy horizon where determinism breaks down. Although infinities are avoided, for all practical purposes the core of the black hole plays the role of a naked singularity. Recent developments in loop quantum gravity indicate that this aggravated information loss problem is likely to be the generic outcome, putting strong conceptual pressure on the theory.
17 pages, 1 figure; v2: new footnotes, new appendices, new references, new question mark
References in corpus (10)
- Quantum Nature of the Big Bang
- Black hole evaporation: A paradigm
- Black holes in loop quantum gravity: the complete space-time
- Spherically Symmetric Quantum Geometry: States and Basic Operators
- Anomaly freedom in perturbative loop quantum gravity
- Non-marginal LTB-like models with inverse triad corrections from loop quantum gravity
- Effective Constraints for Quantum Systems
- Non-Paradoxical Loss of Information in Black Hole Evaporation in a Quantum Collapse Model
- Spherically symmetric canonical quantum gravity
- Fluctuation energies in quantum cosmology
Cited by in corpus (7)
- Hypersurface-deformation algebroids and effective space-time models
- Loop Quantum Gravity
- Linking loop quantum gravity quantization ambiguities with phenomenology
- Brief review on black hole loop quantization
- Effective Field Theory of Loop Quantum Cosmology
- Schrödinger-like quantum dynamics in loop quantized black holes
- Black-hole models in loop quantum gravity