An Overview of Quasinormal Modes in Modified and Extended Gravity

As gravitational waves are now being nearly routinely measured with interferometers, the question of using them to probe new physics becomes increasingly legitimate. In this article, we rely on a well established framework to investigate how the complex frequencies of quasinormal modes are affected...

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Main Authors: Flora Moulin, Aurélien Barrau, Killian Martineau
Format: Article
Language:English
Published: MDPI AG 2019-09-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/5/9/202
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author Flora Moulin
Aurélien Barrau
Killian Martineau
author_facet Flora Moulin
Aurélien Barrau
Killian Martineau
author_sort Flora Moulin
collection DOAJ
description As gravitational waves are now being nearly routinely measured with interferometers, the question of using them to probe new physics becomes increasingly legitimate. In this article, we rely on a well established framework to investigate how the complex frequencies of quasinormal modes are affected by different models. The tendencies are explicitly shown for both the pulsation and the damping rate. The goal is, at this stage, purely qualitative. This opportunity is also taken to derive the Regge-Wheeler equation for general static and spherically symmetric metrics.
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spelling doaj.art-1c3d5354cfee4212a2707050977136fb2022-12-22T04:22:25ZengMDPI AGUniverse2218-19972019-09-015920210.3390/universe5090202universe5090202An Overview of Quasinormal Modes in Modified and Extended GravityFlora Moulin0Aurélien Barrau1Killian Martineau2Laboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3 53, avenue des Martyrs, CEDEX, 38026 Grenoble, FranceLaboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3 53, avenue des Martyrs, CEDEX, 38026 Grenoble, FranceLaboratoire de Physique Subatomique et de Cosmologie, Université Grenoble-Alpes, CNRS/IN2P3 53, avenue des Martyrs, CEDEX, 38026 Grenoble, FranceAs gravitational waves are now being nearly routinely measured with interferometers, the question of using them to probe new physics becomes increasingly legitimate. In this article, we rely on a well established framework to investigate how the complex frequencies of quasinormal modes are affected by different models. The tendencies are explicitly shown for both the pulsation and the damping rate. The goal is, at this stage, purely qualitative. This opportunity is also taken to derive the Regge-Wheeler equation for general static and spherically symmetric metrics.https://www.mdpi.com/2218-1997/5/9/202black holesquasinormal modesgravitationnel wavesmodified gravity
spellingShingle Flora Moulin
Aurélien Barrau
Killian Martineau
An Overview of Quasinormal Modes in Modified and Extended Gravity
Universe
black holes
quasinormal modes
gravitationnel waves
modified gravity
title An Overview of Quasinormal Modes in Modified and Extended Gravity
title_full An Overview of Quasinormal Modes in Modified and Extended Gravity
title_fullStr An Overview of Quasinormal Modes in Modified and Extended Gravity
title_full_unstemmed An Overview of Quasinormal Modes in Modified and Extended Gravity
title_short An Overview of Quasinormal Modes in Modified and Extended Gravity
title_sort overview of quasinormal modes in modified and extended gravity
topic black holes
quasinormal modes
gravitationnel waves
modified gravity
url https://www.mdpi.com/2218-1997/5/9/202
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