Black hole spectroscopy: from theory to experiment
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arXiv
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| 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 |