Hyperboloidal Approach to Quasinormal Modes

Fuente: arXiv
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Autori principali: Macedo, Rodrigo Panosso, Zenginoglu, Anil
Natura: Preprint
Pubblicazione: 2024
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author Macedo, Rodrigo Panosso
Zenginoglu, Anil
author_facet Macedo, Rodrigo Panosso
Zenginoglu, Anil
contents Oscillations of black hole spacetimes exhibit divergent behavior toward the bifurcation sphere and spatial infinity. This divergence can be understood as a consequence of the geometry in these spacetime regions. In contrast, black-hole oscillations are regular when evaluated toward the event horizon and null infinity. Hyperboloidal surfaces naturally connect these regions, providing a geometric regularization of time-harmonic oscillations called quasinormal modes (QNMs). This review traces the historical development of the hyperboloidal approach to QNMs. We discuss the physical motivation for the hyperboloidal approach and highlight current developments in the field.
format Preprint
id arxiv_https___arxiv_org_abs_2409_11478
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Hyperboloidal Approach to Quasinormal Modes
Macedo, Rodrigo Panosso
Zenginoglu, Anil
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Mathematical Physics
Oscillations of black hole spacetimes exhibit divergent behavior toward the bifurcation sphere and spatial infinity. This divergence can be understood as a consequence of the geometry in these spacetime regions. In contrast, black-hole oscillations are regular when evaluated toward the event horizon and null infinity. Hyperboloidal surfaces naturally connect these regions, providing a geometric regularization of time-harmonic oscillations called quasinormal modes (QNMs). This review traces the historical development of the hyperboloidal approach to QNMs. We discuss the physical motivation for the hyperboloidal approach and highlight current developments in the field.
title Hyperboloidal Approach to Quasinormal Modes
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
Mathematical Physics
url https://arxiv.org/abs/2409.11478