Related papers: Fishing massive black hole binaries with THAMES

Optimized Search for a Binary Black Hole Merger Population in LIGO-Virgo O3 Data

Maximizing the number of detections in matched filter searches for compact binary coalescence (CBC) gravitational wave (GW) signals requires a model of the source population distribution. In previous searches using the PyCBC framework,…

General Relativity and Quantum Cosmology · Physics 2024-12-13 Praveen Kumar , Thomas Dent

Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run

This paper reports on an unmodeled, all-sky search for gravitational waves from merging intermediate mass black hole binaries (IMBHB). The search was performed on data from the second joint science run of the LIGO and Virgo detectors (July…

General Relativity and Quantum Cosmology · Physics 2018-09-17 The LIGO Scientific Collaboration , the Virgo Collaboration , J. Aasi , B. P. Abbott , R. Abbott , T. Abbott , M. R. Abernathy , T. Accadia , F. Acernese , K. Ackley , C. Adams , T. Adams , P. Addesso , R. X. Adhikari , C. Affeldt , M. Agathos , N. Aggarwal , O. D. Aguiar , A. Ain , P. Ajith , A. Alemic , B. Allen , A. Allocca , D. Amariutei , M. Andersen , R. Anderson , S. B. Anderson , W. G. Anderson , K. Arai , M. C. Araya , C. Arceneaux , J. Areeda , S. M. Aston , P. Astone , P. Aufmuth , C. Aulbert , L. Austin , B. E. Aylott , S. Babak , P. T. Baker , G. Ballardin , S. W. Ballmer , J. C. Barayoga , M. Barbet , B. C. Barish , D. Barker , F. Barone , B. Barr , L. Barsotti , M. Barsuglia , M. A. Barton , I. Bartos , R. Bassiri , A. Basti , J. C. Batch , J. Bauchrowitz , Th. S. Bauer , V. Bavigadda , B. Behnke , M. Bejger , M. G. Beker , C. Belczynski , A. S. Bell , C. Bell , G. Bergmann , D. Bersanetti , A. Bertolini , J. Betzwieser , P. T. Beyersdorf , I. A. Bilenko , G. Billingsley , J. Birch , S. Biscans , M. Bitossi , M. A. Bizouard , E. Black , J. K. Blackburn , L. Blackburn , D. Blair , S. Bloemen , M. Blom , O. Bock , T. P. Bodiya , M. Boer , G. Bogaert , C. Bogan , C. Bond , F. Bondu , L. Bonelli , R. Bonnand , R. Bork , M. Born , V. Boschi , Sukanta Bose , L. Bosi , C. Bradaschia , P. R. Brady , V. B. Braginsky , M. Branchesi , J. E. Brau , T. Briant , D. O. Bridges , A. Brillet , M. Brinkmann , V. Brisson , A. F. Brooks , D. A. Brown , D. D. Brown , F. Brückner , S. Buchman , T. Bulik , H. J. Bulten , A. Buonanno , R. Burman , D. Buskulic , C. Buy , L. Cadonati , G. Cagnoli , J. Calderón Bustillo , E. Calloni , J. B. Camp , P. Campsie , K. C. Cannon , B. Canuel , J. Cao , C. D. Capano , F. Carbognani , L. Carbone , S. Caride , A. Castiglia , S. Caudill , M. Cavaglià , F. Cavalier , R. Cavalieri , C. Celerier , G. Cella , C. Cepeda , E. Cesarini , R. Chakraborty , T. Chalermsongsak , S. J. Chamberlin , S. Chao , P. Charlton , E. Chassande-Mottin , X. Chen , Y. Chen , A. Chincarini , A. Chiummo , H. S. Cho , J. Chow , N. Christensen , Q. Chu , S. S. Y. Chua , S. Chung , G. Ciani , F. Clara , J. A. Clark , F. Cleva , E. Coccia , P. -F. Cohadon , A. Colla , C. Collette , M. Colombini , L. Cominsky , M. Constancio , A. Conte , D. Cook , T. R. Corbitt , M. Cordier , N. Cornish , A. Corpuz , A. Corsi , C. A. Costa , M. W. Coughlin , S. Coughlin , J. -P. Coulon , S. Countryman , P. Couvares , D. M. Coward , M. Cowart , D. C. Coyne , R. Coyne , K. Craig , J. D. E. Creighton , S. G. Crowder , A. Cumming , L. Cunningham , E. Cuoco , K. Dahl , T. Dal Canton , M. Damjanic , S. L. Danilishin , S. D'Antonio , K. Danzmann , V. Dattilo , H. Daveloza , M. Davier , G. S. Davies , E. J. Daw , R. Day , T. Dayanga , G. Debreczeni , J. Degallaix , S. Deléglise , W. Del Pozzo , T. Denker , T. Dent , H. Dereli , V. Dergachev , R. De Rosa , R. T. DeRosa , R. DeSalvo , S. Dhurandhar , M. Díaz , L. Di Fiore , A. Di Lieto , I. Di Palma , A. Di Virgilio , A. Donath , F. Donovan , K. L. Dooley , S. Doravari , S. Dossa , R. Douglas , T. P. Downes , M. Drago , R. W. P. Drever , J. C. Driggers , Z. Du , M. Ducrot , S. Dwyer , T. Eberle , T. Edo , M. Edwards , A. Effler , H. Eggenstein , P. Ehrens , J. Eichholz , S. S. Eikenberry , G. Endrőczi , R. Essick , T. Etzel , M. Evans , T. Evans , M. Factourovich , V. Fafone , S. Fairhurst , Q. Fang , S. Farinon , B. Farr , W. M. Farr , M. Favata , H. Fehrmann , M. M. Fejer , D. Feldbaum , F. Feroz , I. Ferrante , F. Ferrini , F. Fidecaro , L. S. Finn , I. Fiori , R. P. Fisher , R. Flaminio , J. -D. Fournier , S. Franco , S. Frasca , F. Frasconi , M. Frede , Z. Frei , A. Freise , R. Frey , T. T. Fricke , P. Fritschel , V. V. Frolov , P. Fulda , M. Fyffe , J. Gair , L. Gammaitoni , S. Gaonkar , F. Garufi , N. Gehrels , G. Gemme , E. Genin , A. Gennai , S. Ghosh , J. A. Giaime , K. D. Giardina , A. Giazotto , C. Gill , J. Gleason , E. Goetz , R. Goetz , L. Gondan , G. González , N. Gordon , M. L. Gorodetsky , S. Gossan , S. Goßler , R. Gouaty , C. Gräf , P. B. Graff , M. Granata , A. Grant , S. Gras , C. Gray , R. J. S. Greenhalgh , A. M. Gretarsson , P. Groot , H. Grote , K. Grover , S. Grunewald , G. M. Guidi , C. Guido , K. Gushwa , E. K. Gustafson , R. Gustafson , D. Hammer , G. Hammond , M. Hanke , J. Hanks , C. Hanna , J. Hanson , J. Harms , G. M. Harry , I. W. Harry , E. D. Harstad , M. Hart , M. T. Hartman , C. -J. Haster , K. Haughian , A. Heidmann , M. Heintze , H. Heitmann , P. Hello , G. Hemming , M. Hendry , I. S. Heng , A. W. Heptonstall , M. Heurs , M. Hewitson , S. Hild , D. Hoak , K. A. Hodge , K. Holt , S. Hooper , P. Hopkins , D. J. Hosken , J. Hough , E. J. Howell , Y. Hu , E. Huerta , B. Hughey , S. Husa , S. H. Huttner , M. Huynh , T. Huynh-Dinh , D. R. Ingram , R. Inta , T. Isogai , A. Ivanov , B. R. Iyer , K. Izumi , M. Jacobson , E. James , H. Jang , P. Jaranowski , Y. Ji , F. Jiménez-Forteza , W. W. Johnson , D. I. Jones , R. Jones , R. J. G. Jonker , L. Ju , K Haris , P. Kalmus , V. Kalogera , S. Kandhasamy , G. Kang , J. B. Kanner , J. Karlen , M. Kasprzack , E. Katsavounidis , W. Katzman , H. Kaufer , K. Kawabe , F. Kawazoe , F. Kéfélian , G. M. Keiser , D. Keitel , D. B. Kelley , W. Kells , A. Khalaidovski , F. Y. Khalili , E. A. Khazanov , C. Kim , K. Kim , N. G. Kim , N. Kim , Y. -M. Kim , E. J. King , P. J. King , D. L. Kinzel , J. S. Kissel , S. Klimenko , J. Kline , S. Koehlenbeck , K. Kokeyama , V. Kondrashov , S. Koranda , W. Z. Korth , I. Kowalska , D. B. Kozak , A. Kremin , V. Kringel , B. Krishnan , A. Królak , G. Kuehn , A. Kumar , P. Kumar , R. Kumar , L. Kuo , A. Kutynia , P. Kwee , M. Landry , B. Lantz , S. Larson , P. D. Lasky , C. Lawrie , A. Lazzarini , C. Lazzaro , P. Leaci , S. Leavey , E. O. Lebigot , C. -H. Lee , H. K. Lee , H. M. Lee , J. Lee , M. Leonardi , J. R. Leong , A. Le Roux , N. Leroy , N. Letendre , Y. Levin , B. Levine , J. Lewis , T. G. F. Li , K. Libbrecht , A. Libson , A. C. Lin , T. B. Littenberg , V. Litvine , N. A. Lockerbie , V. Lockett , D. Lodhia , K. Loew , J. Logue , A. L. Lombardi , M. Lorenzini , V. Loriette , M. Lormand , G. Losurdo , J. Lough , M. J. Lubinski , H. Lück , E. Luijten , A. P. Lundgren , R. Lynch , Y. Ma , J. Macarthur , E. P. Macdonald , T. MacDonald , B. Machenschalk , M. MacInnis , D. M. Macleod , F. Magana-Sandoval , M. Mageswaran , C. Maglione , K. Mailand , E. Majorana , I. Maksimovic , V. Malvezzi , N. Man , G. M. Manca , I. Mandel , V. Mandic , V. Mangano , N. Mangini , M. Mantovani , F. Marchesoni , F. Marion , S. Márka , Z. Márka , A. Markosyan , E. Maros , J. Marque , F. Martelli , I. W. Martin , R. M. Martin , L. Martinelli , D. Martynov , J. N. Marx , K. Mason , A. Masserot , T. J. Massinger , F. Matichard , L. Matone , R. A. Matzner , N. Mavalvala , N. Mazumder , G. Mazzolo , R. McCarthy , D. E. McClelland , S. C. McGuire , G. McIntyre , J. McIver , K. McLin , D. Meacher , G. D. Meadors , M. Mehmet , J. Meidam , M. Meinders , A. Melatos , G. Mendell , R. A. Mercer , S. Meshkov , C. Messenger , P. Meyers , H. Miao , C. Michel , E. E. Mikhailov , L. Milano , S. Milde , J. Miller , Y. Minenkov , C. M. F. Mingarelli , C. Mishra , S. Mitra , V. P. Mitrofanov , G. Mitselmakher , R. Mittleman , B. Moe , P. Moesta , A. Moggi , M. Mohan , S. R. P. Mohapatra , D. Moraru , G. Moreno , N. Morgado , S. R. Morriss , K. Mossavi , B. Mours , C. M. Mow-Lowry , C. L. Mueller , G. Mueller , S. Mukherjee , A. Mullavey , J. Munch , D. Murphy , P. G. Murray , A. Mytidis , M. F. Nagy , D. Nanda Kumar , I. Nardecchia , L. Naticchioni , R. K. Nayak , V. Necula , G. Nelemans , I. Neri , M. Neri , G. Newton , T. Nguyen , A. Nitz , F. Nocera , D. Nolting , M. E. N. Normandin , L. K. Nuttall , E. Ochsner , J. O'Dell , E. Oelker , J. J. Oh , S. H. Oh , F. Ohme , P. Oppermann , B. O'Reilly , R. O'Shaughnessy , C. Osthelder , D. J. Ottaway , R. S. Ottens , H. Overmier , B. J. Owen , C. Padilla , A. Pai , O. Palashov , C. Palomba , H. Pan , Y. Pan , C. Pankow , F. Paoletti , M. A. Papa , H. Paris , A. Pasqualetti , R. Passaquieti , D. Passuello , M. Pedraza , S. Penn , A. Perreca , M. Phelps , M. Pichot , M. Pickenpack , F. Piergiovanni , V. Pierro , L. Pinard , I. M. Pinto , M. Pitkin , J. Poeld , R. Poggiani , A. Poteomkin , J. Powell , J. Prasad , S. Premachandra , T. Prestegard , L. R. Price , M. Prijatelj , S. Privitera , G. A. Prodi , L. Prokhorov , O. Puncken , M. Punturo , P. Puppo , J. Qin , V. Quetschke , E. Quintero , G. Quiroga , R. Quitzow-James , F. J. Raab , D. S. Rabeling , I. Rácz , H. Radkins , P. Raffai , S. Raja , G. Rajalakshmi , M. Rakhmanov , C. Ramet , K. Ramirez , P. Rapagnani , V. Raymond , V. Re , J. Read , C. M. Reed , T. Regimbau , S. Reid , D. H. Reitze , E. Rhoades , F. Ricci , K. Riles , N. A. Robertson , F. Robinet , A. Rocchi , M. Rodruck , L. Rolland , J. G. Rollins , R. Romano , G. Romanov , J. H. Romie , D. Rosińska , S. Rowan , A. Rüdiger , P. Ruggi , K. Ryan , F. Salemi , L. Sammut , V. Sandberg , J. R. Sanders , V. Sannibale , I. Santiago-Prieto , E. Saracco , B. Sassolas , B. S. Sathyaprakash , P. R. Saulson , R. Savage , J. Scheuer , R. Schilling , R. Schnabel , R. M. S. Schofield , E. Schreiber , D. Schuette , B. F. Schutz , J. Scott , S. M. Scott , D. Sellers , A. S. Sengupta , D. Sentenac , V. Sequino , A. Sergeev , D. Shaddock , S. Shah , M. S. Shahriar , M. Shaltev , B. Shapiro , P. Shawhan , D. H. Shoemaker , T. L. Sidery , K. Siellez , X. Siemens , D. Sigg , D. Simakov , A. Singer , L. Singer , R. Singh , A. M. Sintes , B. J. J. Slagmolen , J. Slutsky , J. R. Smith , M. Smith , R. J. E. Smith , N. D. Smith-Lefebvre , E. J. Son , B. Sorazu , T. Souradeep , A. Staley , J. Stebbins , J. Steinlechner , S. Steinlechner , B. C. Stephens , S. Steplewski , S. Stevenson , R. Stone , D. Stops , K. A. Strain , N. Straniero , S. Strigin , R. Sturani , A. L. Stuver , T. Z. Summerscales , S. Susmithan , P. J. Sutton , B. Swinkels , M. Tacca , D. Talukder , D. B. Tanner , S. P. Tarabrin , R. Taylor , A. P. M. ter Braack , M. P. Thirugnanasambandam , M. Thomas , P. Thomas , K. A. Thorne , K. S. Thorne , E. Thrane , V. Tiwari , K. V. Tokmakov , C. Tomlinson , M. Tonelli , C. V. Torres , C. I. Torrie , F. Travasso , G. Traylor , M. Tse , D. Ugolini , C. S. Unnikrishnan , A. L. Urban , K. Urbanek , H. Vahlbruch , G. Vajente , G. Valdes , M. Vallisneri , M. van Beuzekom , J. F. J. van den Brand , C. Van Den Broeck , S. van der Putten , M. V. van der Sluys , J. van Heijningen , A. A. van Veggel , S. Vass , M. Vasúth , R. Vaulin , A. Vecchio , G. Vedovato , J. Veitch , P. J. Veitch , K. Venkateswara , D. Verkindt , S. S. Verma , F. Vetrano , A. Viceré , R. Vincent-Finley , J. -Y. Vinet , S. Vitale , T. Vo , H. Vocca , C. Vorvick , W. D. Vousden , S. P. Vyachanin , A. Wade , L. Wade , M. Wade , M. Walker , L. Wallace , M. Wang , X. Wang , R. L. Ward , M. Was , B. Weaver , L. -W. Wei , M. Weinert , A. J. Weinstein , R. Weiss , T. Welborn , L. Wen , P. Wessels , M. West , T. Westphal , K. Wette , J. T. Whelan , D. J. White , B. F. Whiting , K. Wiesner , C. Wilkinson , K. Williams , L. Williams , R. Williams , T. Williams , A. R. Williamson , J. L. Willis , B. Willke , M. Wimmer , W. Winkler , C. C. Wipf , A. G. Wiseman , H. Wittel , G. Woan , J. Worden , J. Yablon , I. Yakushin , H. Yamamoto , C. C. Yancey , H. Yang , Z. Yang , S. Yoshida , M. Yvert , A. Zadrożny , M. Zanolin , J. -P. Zendri , Fan Zhang , L. Zhang , C. Zhao , X. J. Zhu , M. E. Zucker , S. Zuraw , J. Zweizig

Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope

Gravitational-wave (GW) detection offers a novel approach to exploring intermediate-mass black holes (IMBHs). The GW signals from IMBH mergers mainly fall in the decihertz frequency band. The lunar-based GW detector, the Lunar…

General Relativity and Quantum Cosmology · Physics 2026-03-18 Yue-Yan Dong , Ji-Yu Song , Jing-Fei Zhang , Xin Zhang

The High-Mass-Ratio Challenge in Gravitational Waveform Modelling

Binary black hole (BBH) mergers detected via gravitational waves are addressing key open questions in astrophysics, cosmology, and fundamental physics. Our scientific conclusions rely on extracting accurate source parameters, for which we…

General Relativity and Quantum Cosmology · Physics 2026-03-30 Parthapratim Mahapatra , Jonathan E. Thompson , Edward Fauchon-Jones , Mark Hannam

On the detectability of higher harmonics with LISA

Supermassive black hole binaries (SMBHBs) are expected to be detected by the future space-based gravitational-wave detector LISA with a large signal-to-noise ratio (SNR). This prospect enhances the possibility of differentiating higher…

General Relativity and Quantum Cosmology · Physics 2024-10-01 Chantal Pitte , Quentin Baghi , Sylvain Marsat , Marc Besançon , Antoine Petiteau

Detection and Prediction of Future Massive Black Hole Mergers with Machine Learning and Truncated Waveforms

We present a novel machine learning framework tailored to detect massive black hole binaries observed by spaceborne gravitational wave detectors like the Laser Interferometer Space Antenna (LISA) and predict their future merger times. The…

Instrumentation and Methods for Astrophysics · Physics 2024-05-21 Niklas Houba , Stefan H. Strub , Luigi Ferraioli , Domenico Giardini

Deep Learning Detection and Classification of Gravitational Waves from Neutron Star-Black Hole Mergers

The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo Interferometer Collaborations have now detected all three classes of compact binary mergers: binary black hole (BBH), binary neutron star (BNS), and neutron star-black…

Instrumentation and Methods for Astrophysics · Physics 2023-03-20 Richard Qiu , Plamen Krastev , Kiranjyot Gill , Edo Berger

A Higher Probability of Detecting Lensed Supermassive Black Hole Binaries by LISA

Gravitational lensing of gravitational waves (GWs) is a powerful probe of the matter distribution in the universe. Here we revisit the wave-optics effects induced by dark matter (DM) halos on the GW signals of merging massive black hole…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-23 Zucheng Gao , Xian Chen , Yi-Ming Hu , Jian-Dong Zhang , Shunjia Huang

Detecting Intermediate-Mass Ratio Inspirals From The Ground And Space

The detection of a gravitational capture of a stellar-mass compact object by a massive black hole (MBH) will allow us to test gravity in the strong regime. These sources form via two-body relaxation, by exchanging energy and angular…

High Energy Astrophysical Phenomena · Physics 2018-10-03 Pau Amaro-Seoane

Parameter Distributions of Binary Black Hole Mergers Near Supermassive Black Holes as Seen by Advanced Gravitational Wave Detectors

The environment surrounding supermassive black holes (SMBHs) in galactic nuclei (GNs) is expected to harbour stellar-mass binary black hole (BBH) populations. These binaries were suggested to form a hierarchical triple system with the SMBH,…

High Energy Astrophysical Phenomena · Physics 2022-12-21 László Gondán

Detecting Black-Hole Binary Clustering via the Second-Generation Gravitational-Wave Detectors

The first discovery of the gravitational wave (GW) event, GW150914, suggests a higher merger rate of black-hole (BH) binaries. If this is true, a number of BH binaries will be observed via the second-generation GW detectors, and the…

Cosmology and Nongalactic Astrophysics · Physics 2016-07-13 Toshiya Namikawa , Atsushi Nishizawa , Atsushi Taruya

Accessing Intermediate-Mass Black Holes in 728 Globular Star Clusters in NGC\,4472

Intermediate-mass black holes (IMBHs) by definition have masses of $M_{\rm IMBH} \sim 10^{2-5}~M_\odot$, a range with few observational constraints. Finding IMBHs in globular star clusters (GCs) would validate a formation channel for…

Astrophysics of Galaxies · Physics 2021-09-08 J. M. Wrobel , T. J. Maccarone , J. C. A. Miller-Jones , K. E. Nyland

On the detectability of massive black hole merger eventsby LISA

The launch of space based gravitational wave (GW) detectors (e.g. Laser Interferometry Space Antenna; LISA) and current and upcoming Pulsar Timing Arrays (PTAs) will extend the GW window to low frequencies, opening new investigations into…

High Energy Astrophysical Phenomena · Physics 2022-04-20 Samuel Banks , Katharine Lee , Nazanin Azimi , Kendall Scarborough , Nikolai Stefanov , Indra Periwal , Colin DeGraf , Tiziana Di Matteo

Performance of a Chirplet-based analysis for gravitational waves from binary black hole mergers

The gravitational wave (GW) signature of a binary black hole (BBH) coalescence is characterized by rapid frequency evolution in the late inspiral and merger phases. For a system with total mass larger than 100 M_sun, ground based GW…

General Relativity and Quantum Cosmology · Physics 2015-06-03 Satya Mohapatra , Zachary Nemtzow , Eric Chassande-Mottin , Laura Cadonati

What we can learn from multi-band observations of black hole binaries

The LIGO/Virgo gravitational-wave (GW) interferometers have to-date detected ten merging black hole (BH) binaries, some with masses considerably larger than had been anticipated. Stellar-mass BH binaries at the high end of the observed mass…

High Energy Astrophysical Phenomena · Physics 2019-03-12 Curt Cutler , Emanuele Berti , Karan Jani , Ely D. Kovetz , Lisa Randall , Salvatore Vitale , Kaze W. K. Wong , Kelly Holley-Bockelmann , Shane L. Larson , Tyson Littenberg , Sean T. McWilliams , Guido Mueller , Jeremy D. Schnittman , David H. Shoemaker , Michele Vallisneri

Rapid search for massive black hole binary coalescences using deep learning

The coalescences of massive black hole binaries are one of the main targets of space-based gravitational wave observatories. Such gravitational wave sources are expected to be accompanied by electromagnetic emissions. Low latency detection…

Instrumentation and Methods for Astrophysics · Physics 2023-04-18 Wen-Hong Ruan , He Wang , Chang Liu , Zong-Kuan Guo

Eccentric Pairs: Analytic Gravitational Waves from Binary Black Holes in Elliptic Orbits

Gravitational waves (GW) from eccentric binaries have intricate signals encoding important features about the location, creation and evolution of the sources. Eccentricity shortens the merger time, making the emitted GW statistically…

General Relativity and Quantum Cosmology · Physics 2024-05-13 Dillon Buskirk , Maria C. Babiuc Hamilton

Low-frequency gravitational radiation from coalescing massive black hole binaries in hierarchical cosmologies

We compute the expected gravitational wave signal from coalescing massive black hole (MBH) binaries at the center of galaxies in a hierarchical structure formation scenario in which seed holes of intermediate mass form far up in the dark…

Astrophysics · Physics 2009-11-10 Alberto Sesana , Francesco Haardt , Piero Madau , Marta Volonteri

Study of the Intermediate Mass Ratio Black Hole Binary Merger up to 1000:1 with Numerical Relativity

We explicitly demonstrate that current numerical relativity techniques are able to accurately evolve black hole binaries with mass ratios of the order of 1000:1. This proof of principle is relevant for future third generation (3G)…

General Relativity and Quantum Cosmology · Physics 2023-04-19 Carlos O. Lousto , James Healy

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers

Next-generation ground-based gravitational wave observatories will observe mergers of intermediate-mass black holes (IMBHs) out to high redshift. Such IMBHs can form through runaway tidal encounters in the cores of dense stellar clusters.…

High Energy Astrophysical Phenomena · Physics 2025-03-27 Konstantinos Kritos , Luca Reali , Ken K. Y. Ng , Fabio Antonini , Emanuele Berti