Gravitational Waves from Black Hole Emission

Using adiabatic point-particle black hole perturbation theory, we simulate plausible gravitational wave (GW) signatures in two exotic scenarios (i) where a small black hole is emitted by a larger one (‘black hole emission’) and (ii) where a small black hole is emitted by a larger one and subsequentl...

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Main Authors: Tousif Islam, Gaurav Khanna, Steven L. Liebling
Format: Article
Language:English
Published: MDPI AG 2025-01-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/11/1/21
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author Tousif Islam
Gaurav Khanna
Steven L. Liebling
author_facet Tousif Islam
Gaurav Khanna
Steven L. Liebling
author_sort Tousif Islam
collection DOAJ
description Using adiabatic point-particle black hole perturbation theory, we simulate plausible gravitational wave (GW) signatures in two exotic scenarios (i) where a small black hole is emitted by a larger one (‘black hole emission’) and (ii) where a small black hole is emitted by a larger one and subsequently absorbed back (‘black hole absorption’). While such scenarios are forbidden in general relativity (GR), alternative theories (such as certain quantum gravity scenarios obeying the weak gravity conjecture, white holes, and Hawking radiation) may allow them. By leveraging the phenomenology of black hole emission and absorption signals, we introduce straightforward modifications to existing gravitational waveform models to mimic gravitational radiation associated with these exotic events. We anticipate that these (incomplete but) initial simulations, coupled with the adjusted waveform models, will aid in the development of null tests for GR using GWs.
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spelling doaj-art-f0e5809ebd434f628d3c021cae30ba922025-01-24T13:51:30ZengMDPI AGUniverse2218-19972025-01-011112110.3390/universe11010021Gravitational Waves from Black Hole EmissionTousif Islam0Gaurav Khanna1Steven L. Liebling2Kavli Institute of Theoretical Physics, University of California Santa Barbara, Santa Barbara, CA 93106, USADepartment of Physics, University of Massachusetts, Dartmouth, MA 02747, USASchool of Natural and Life Sciences, Long Island University, Brookville, NY 11548, USAUsing adiabatic point-particle black hole perturbation theory, we simulate plausible gravitational wave (GW) signatures in two exotic scenarios (i) where a small black hole is emitted by a larger one (‘black hole emission’) and (ii) where a small black hole is emitted by a larger one and subsequently absorbed back (‘black hole absorption’). While such scenarios are forbidden in general relativity (GR), alternative theories (such as certain quantum gravity scenarios obeying the weak gravity conjecture, white holes, and Hawking radiation) may allow them. By leveraging the phenomenology of black hole emission and absorption signals, we introduce straightforward modifications to existing gravitational waveform models to mimic gravitational radiation associated with these exotic events. We anticipate that these (incomplete but) initial simulations, coupled with the adjusted waveform models, will aid in the development of null tests for GR using GWs.https://www.mdpi.com/2218-1997/11/1/21black holesgravitational wavesperturbation theorybinary systemsgeneral relativityTeukolsky equation
spellingShingle Tousif Islam
Gaurav Khanna
Steven L. Liebling
Gravitational Waves from Black Hole Emission
Universe
black holes
gravitational waves
perturbation theory
binary systems
general relativity
Teukolsky equation
title Gravitational Waves from Black Hole Emission
title_full Gravitational Waves from Black Hole Emission
title_fullStr Gravitational Waves from Black Hole Emission
title_full_unstemmed Gravitational Waves from Black Hole Emission
title_short Gravitational Waves from Black Hole Emission
title_sort gravitational waves from black hole emission
topic black holes
gravitational waves
perturbation theory
binary systems
general relativity
Teukolsky equation
url https://www.mdpi.com/2218-1997/11/1/21
work_keys_str_mv AT tousifislam gravitationalwavesfromblackholeemission
AT gauravkhanna gravitationalwavesfromblackholeemission
AT stevenlliebling gravitationalwavesfromblackholeemission