Black hole spectroscopy: from theory to experiment

Fuente: arXiv
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Main Authors: Berti, Emanuele, Cardoso, Vitor, Carullo, Gregorio, Abedi, Jahed, Afshordi, Niayesh, Albanesi, Simone, Baibhav, Vishal, Bhagwat, Swetha, Blázquez-Salcedo, José Luis, Bonga, Béatrice, Bucciotti, Bruno, Santoro, Giada Caneva, Cano, Pablo A., Capano, Collin, Cheung, Mark Ho-Yeuk, Chirenti, Cecilia, Cook, Gregory B., Chung, Adrian Ka-Wai, De Amicis, Marina, Destounis, Kyriakos, Dias, Oscar J. C., Del Pozzo, Walter, Duque, Francisco, Farr, Will M., Finch, Eliot, Franchini, Nicola, Fransen, Kwinten, Gennari, Vasco, Green, Stephen R., Hughes, Scott A., Isi, Maximiliano, Forteza, Xisco Jimenez, Khanna, Gaurav, Khoo, Fech Scen, Kimura, Masashi, Krishnan, Badri, Kuntz, Adrien, Lagos, Macarena, Lo, Rico K. L., London, Lionel, Ma, Sizheng, Maenaut, Simon, Zertuche, Lorena Magaña, Maggio, Elisa, Maselli, Andrea, Mitman, Keefe, Motohashi, Hayato, Oshita, Naritaka, Pacilio, Costantino, Pani, Paolo, Macedo, Rodrigo Panosso, Pitte, Chantal, Pompili, Lorenzo, Redondo-Yuste, Jaime, Richartz, Maurício, Riotto, Antonio, Santos, Jorge E., Sathyaprakash, Bangalore, Sberna, Laura, Silva, Hector O., Stein, Leo C., Toubiana, Alexandre, Völkel, Sebastian H., Westerweck, Julian, Yang, Huan, Yi, Sophia, Yunes, Nicolas, Zhu, Hengrui
Format: Preprint
Published: 2025
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author Berti, Emanuele
Cardoso, Vitor
Carullo, Gregorio
Abedi, Jahed
Afshordi, Niayesh
Albanesi, Simone
Baibhav, Vishal
Bhagwat, Swetha
Blázquez-Salcedo, José Luis
Bonga, Béatrice
Bucciotti, Bruno
Santoro, Giada Caneva
Cano, Pablo A.
Capano, Collin
Cheung, Mark Ho-Yeuk
Chirenti, Cecilia
Cook, Gregory B.
Chung, Adrian Ka-Wai
De Amicis, Marina
Destounis, Kyriakos
Dias, Oscar J. C.
Del Pozzo, Walter
Duque, Francisco
Farr, Will M.
Finch, Eliot
Franchini, Nicola
Fransen, Kwinten
Gennari, Vasco
Green, Stephen R.
Hughes, Scott A.
Isi, Maximiliano
Forteza, Xisco Jimenez
Khanna, Gaurav
Khoo, Fech Scen
Kimura, Masashi
Krishnan, Badri
Kuntz, Adrien
Lagos, Macarena
Lo, Rico K. L.
London, Lionel
Ma, Sizheng
Maenaut, Simon
Zertuche, Lorena Magaña
Maggio, Elisa
Maselli, Andrea
Mitman, Keefe
Motohashi, Hayato
Oshita, Naritaka
Pacilio, Costantino
Pani, Paolo
Macedo, Rodrigo Panosso
Pitte, Chantal
Pompili, Lorenzo
Redondo-Yuste, Jaime
Richartz, Maurício
Riotto, Antonio
Santos, Jorge E.
Sathyaprakash, Bangalore
Sberna, Laura
Silva, Hector O.
Stein, Leo C.
Toubiana, Alexandre
Völkel, Sebastian H.
Westerweck, Julian
Yang, Huan
Yi, Sophia
Yunes, Nicolas
Zhu, Hengrui
author_facet Berti, Emanuele
Cardoso, Vitor
Carullo, Gregorio
Abedi, Jahed
Afshordi, Niayesh
Albanesi, Simone
Baibhav, Vishal
Bhagwat, Swetha
Blázquez-Salcedo, José Luis
Bonga, Béatrice
Bucciotti, Bruno
Santoro, Giada Caneva
Cano, Pablo A.
Capano, Collin
Cheung, Mark Ho-Yeuk
Chirenti, Cecilia
Cook, Gregory B.
Chung, Adrian Ka-Wai
De Amicis, Marina
Destounis, Kyriakos
Dias, Oscar J. C.
Del Pozzo, Walter
Duque, Francisco
Farr, Will M.
Finch, Eliot
Franchini, Nicola
Fransen, Kwinten
Gennari, Vasco
Green, Stephen R.
Hughes, Scott A.
Isi, Maximiliano
Forteza, Xisco Jimenez
Khanna, Gaurav
Khoo, Fech Scen
Kimura, Masashi
Krishnan, Badri
Kuntz, Adrien
Lagos, Macarena
Lo, Rico K. L.
London, Lionel
Ma, Sizheng
Maenaut, Simon
Zertuche, Lorena Magaña
Maggio, Elisa
Maselli, Andrea
Mitman, Keefe
Motohashi, Hayato
Oshita, Naritaka
Pacilio, Costantino
Pani, Paolo
Macedo, Rodrigo Panosso
Pitte, Chantal
Pompili, Lorenzo
Redondo-Yuste, Jaime
Richartz, Maurício
Riotto, Antonio
Santos, Jorge E.
Sathyaprakash, Bangalore
Sberna, Laura
Silva, Hector O.
Stein, Leo C.
Toubiana, Alexandre
Völkel, Sebastian H.
Westerweck, Julian
Yang, Huan
Yi, Sophia
Yunes, Nicolas
Zhu, Hengrui
contents The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes and comparing them with gravitational-wave data from compact binary mergers we can advance our understanding of the two-body problem in general relativity, verify the predictions of the theory in the regime of strong and dynamical gravitational fields, and search for physics beyond the Standard Model or new gravitational degrees of freedom. We summarize the state of the art in our understanding of black hole quasinormal modes in general relativity and modified gravity, their excitation, and the modeling of ringdown waveforms. We also review the status of LIGO-Virgo-KAGRA ringdown observations, data analysis techniques, and the bright prospects of the field in the era of LISA and next-generation ground-based gravitational-wave detectors.
format Preprint
id arxiv_https___arxiv_org_abs_2505_23895
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Black hole spectroscopy: from theory to experiment
Berti, Emanuele
Cardoso, Vitor
Carullo, Gregorio
Abedi, Jahed
Afshordi, Niayesh
Albanesi, Simone
Baibhav, Vishal
Bhagwat, Swetha
Blázquez-Salcedo, José Luis
Bonga, Béatrice
Bucciotti, Bruno
Santoro, Giada Caneva
Cano, Pablo A.
Capano, Collin
Cheung, Mark Ho-Yeuk
Chirenti, Cecilia
Cook, Gregory B.
Chung, Adrian Ka-Wai
De Amicis, Marina
Destounis, Kyriakos
Dias, Oscar J. C.
Del Pozzo, Walter
Duque, Francisco
Farr, Will M.
Finch, Eliot
Franchini, Nicola
Fransen, Kwinten
Gennari, Vasco
Green, Stephen R.
Hughes, Scott A.
Isi, Maximiliano
Forteza, Xisco Jimenez
Khanna, Gaurav
Khoo, Fech Scen
Kimura, Masashi
Krishnan, Badri
Kuntz, Adrien
Lagos, Macarena
Lo, Rico K. L.
London, Lionel
Ma, Sizheng
Maenaut, Simon
Zertuche, Lorena Magaña
Maggio, Elisa
Maselli, Andrea
Mitman, Keefe
Motohashi, Hayato
Oshita, Naritaka
Pacilio, Costantino
Pani, Paolo
Macedo, Rodrigo Panosso
Pitte, Chantal
Pompili, Lorenzo
Redondo-Yuste, Jaime
Richartz, Maurício
Riotto, Antonio
Santos, Jorge E.
Sathyaprakash, Bangalore
Sberna, Laura
Silva, Hector O.
Stein, Leo C.
Toubiana, Alexandre
Völkel, Sebastian H.
Westerweck, Julian
Yang, Huan
Yi, Sophia
Yunes, Nicolas
Zhu, Hengrui
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes and comparing them with gravitational-wave data from compact binary mergers we can advance our understanding of the two-body problem in general relativity, verify the predictions of the theory in the regime of strong and dynamical gravitational fields, and search for physics beyond the Standard Model or new gravitational degrees of freedom. We summarize the state of the art in our understanding of black hole quasinormal modes in general relativity and modified gravity, their excitation, and the modeling of ringdown waveforms. We also review the status of LIGO-Virgo-KAGRA ringdown observations, data analysis techniques, and the bright prospects of the field in the era of LISA and next-generation ground-based gravitational-wave detectors.
title Black hole spectroscopy: from theory to experiment
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2505.23895