Quasinormal modes of loop quantum black holes near the Planck scale
Douglas M. Gingrich

TL;DR
This paper compares quasinormal modes of different loop quantum gravity-inspired black hole metrics near the Planck scale, analyzing perturbations and ringdown behaviors to understand quantum effects on black hole stability.
Contribution
It provides a comparative analysis of axial gravitational quasinormal modes across four loop quantum gravity-inspired black hole models, including time evolution and eikonal limit predictions.
Findings
Differences in quasinormal mode spectra among the models.
Validation of eikonal approximation against numerical results.
Insights into quantum gravity effects on black hole ringdowns.
Abstract
We compare four loop quantum gravity inspired black hole metrics near the Planck scale. Spin 0, 1/2, 1, and 2 field perturbations on these backgrounds are studied. The axial gravitational quasinormal modes are calculated and compared. The time evolution of the ringdown is examined. We also calculate the quasinormal modes in the eikonal limit and compare with the predictions from circular null geodesics.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Pulsars and Gravitational Waves Research · Noncommutative and Quantum Gravity Theories
