相关论文: Length dependence of waveform mismatch: a caveat o…

Calibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914

In Advanced LIGO, detection and astrophysical source parameter estimation of the binary black hole merger GW150914 requires a calibrated estimate of the gravitational-wave strain sensed by the detectors. Producing an estimate from each…

广义相对论与量子宇宙学 · 物理学 2017-04-05 The LIGO Scientific Collaboration , B. P. Abbott , R. Abbott , T. D. Abbott , M. R. Abernathy , K. Ackley , C. Adams , P. Addesso , R. X. Adhikari , V. B. Adya , C. Affeldt , N. Aggarwal , O. D. Aguiar , A. Ain , P. Ajith , B. Allen , P. A. Altin , D. V. Amariutei , S. B. Anderson , W. G. Anderson , K. Arai , M. C. Araya , C. C. Arceneaux , J. S. Areeda , K. G. Arun , G. Ashton , M. Ast , S. M. Aston , P. Aufmuth , C. Aulbert , S. Babak , P. T. Baker , S. W. Ballmer , J. C. Barayoga , S. E. Barclay , B. C. Barish , D. Barker , B. Barr , L. Barsotti , J. Bartlett , I. Bartos , R. Bassiri , J. C. Batch , C. Baune , B. Behnke , A. S. Bell , C. J. Bell , B. K. Berger , J. Bergman , G. Bergmann , C. P. L. Berry , J. Betzwieser , S. Bhagwat , R. Bhandare , I. A. Bilenko , G. Billingsley , J. Birch , R. Birney , S. Biscans , A. Bisht , C. Biwer , J. K. Blackburn , C. D. Blair , D. Blair , R. M. Blair , O. Bock , T. P. Bodiya , C. Bogan , A. Bohe , P. Bojtos , C. Bond , R. Bork , S. Bose , P. R. Brady , V. B. Braginsky , J. E. Brau , M. Brinkmann , P. Brockill , A. F. Brooks , D. A. Brown , D. D. Brown , N. M. Brown , C. C. Buchanan , A. Buikema , A. Buonanno , R. L. Byer , L. Cadonati , C. Cahillane , J. Calderón Bustillo , T. Callister , J. B. Camp , K. C. Cannon , J. Cao , C. D. Capano , S. Caride , S. Caudill , M. Cavaglià , C. Cepeda , R. Chakraborty , T. Chalermsongsak , S. J. Chamberlin , M. Chan , S. Chao , P. Charlton , H. Y. Chen , Y. Chen , C. Cheng , H. S. Cho , M. Cho , J. H. Chow , N. Christensen , Q. Chu , S. Chung , G. Ciani , F. Clara , J. A. Clark , C. G. Collette , L. Cominsky , M. Constancio , D. Cook , T. R. Corbitt , N. Cornish , A. Corsi , C. A. Costa , M. W. Coughlin , S. B. Coughlin , S. T. Countryman , P. Couvares , D. M. Coward , M. J. Cowart , D. C. Coyne , R. Coyne , K. Craig , J. D. E. Creighton , J. Cripe , S. G. Crowder , A. Cumming , L. Cunningham , T. Dal Canton , S. L. Danilishin , K. Danzmann , N. S. Darman , I. Dave , H. P. Daveloza , G. S. Davies , E. J. Daw , D. DeBra , W. Del Pozzo , T. Denker , T. Dent , V. Dergachev , R. DeRosa , R. DeSalvo , S. Dhurandhar , M. C. Díaz , I. Di Palma , G. Dojcinoski , F. Donovan , K. L. Dooley , S. Doravari , R. Douglas , T. P. Downes , M. Drago , R. W. P. Drever , J. C. Driggers , Z. Du , S. E. Dwyer , T. B. Edo , M. C. Edwards , A. Effler , H. -B. Eggenstein , P. Ehrens , J. Eichholz , S. S. Eikenberry , W. Engels , R. C. Essick , T. Etzel , M. Evans , T. M. Evans , R. Everett , M. Factourovich , H. Fair , S. Fairhurst , X. Fan , Q. Fang , B. Farr , W. M. Farr , M. Favata , M. Fays , H. Fehrmann , M. M. Fejer , E. C. Ferreira , R. P. Fisher , M. Fletcher , Z. Frei , A. Freise , R. Frey , T. T. Fricke , P. Fritschel , V. V. Frolov , P. Fulda , M. Fyffe , H. A. G. Gabbard , J. R. Gair , S. G. Gaonkar , G. Gaur , N. Gehrels , J. George , L. Gergely , A. Ghosh , J. A. Giaime , K. D. Giardina , K. Gill , A. Glaefke , E. Goetz , R. Goetz , L. Gondan , G. González , A. Gopakumar , N. A. Gordon , M. L. Gorodetsky , S. E. Gossan , C. Graef , P. B. Graff , A. Grant , S. Gras , C. Gray , A. C. Green , H. Grote , S. Grunewald , X. Guo , A. Gupta , M. K. Gupta , K. E. Gushwa , E. K. Gustafson , R. Gustafson , J. J. Hacker , B. R. Hall , E. D. Hall , G. Hammond , M. Haney , M. M. Hanke , J. Hanks , C. Hanna , M. D. Hannam , J. Hanson , T. Hardwick , G. M. Harry , I. W. Harry , M. J. Hart , M. T. Hartman , C. -J. Haster , K. Haughian , M. C. Heintze , M. Hendry , I. S. Heng , J. Hennig , A. W. Heptonstall , M. Heurs , S. Hild , D. Hoak , K. A. Hodge , S. E. Hollitt , K. Holt , D. E. Holz , P. Hopkins , D. J. Hosken , J. Hough , E. A. Houston , E. J. Howell , Y. M. Hu , S. Huang , E. A. Huerta , B. Hughey , S. Husa , S. H. Huttner , T. Huynh-Dinh , A. Idrisy , N. Indik , D. R. Ingram , R. Inta , H. N. Isa , M. Isi , G. Islas , T. Isogai , B. R. Iyer , K. Izumi , H. Jang , K. Jani , S. Jawahar , F. Jiménez-Forteza , W. W. Johnson , D. I. Jones , R. Jones , L. Ju , Haris K , C. V. Kalaghatgi , V. Kalogera , S. Kandhasamy , G. Kang , J. B. Kanner , S. Karki , M. Kasprzack , E. Katsavounidis , W. Katzman , S. Kaufer , T. Kaur , K. Kawabe , F. Kawazoe , M. S. Kehl , D. Keitel , D. B. Kelley , W. Kells , R. Kennedy , J. S. Key , A. Khalaidovski , F. Y. Khalili , S. Khan , Z. Khan , E. A. Khazanov , N. Kijbunchoo , C. Kim , J. Kim , K. Kim , N. Kim , N. Kim , Y. -M. Kim , E. J. King , P. J. King , D. L. Kinzel , J. S. Kissel , L. Kleybolte , S. Klimenko , S. M. Koehlenbeck , K. Kokeyama , V. Kondrashov , A. Kontos , M. Korobko , W. Z. Korth , D. B. Kozak , V. Kringel , B. Krishnan , C. Krueger , G. Kuehn , P. Kumar , L. Kuo , B. D. Lackey , M. Landry , J. Lange , B. Lantz , P. D. Lasky , A. Lazzarini , C. Lazzaro , P. Leaci , S. Leavey , E. O. Lebigot , C. H. Lee , H. K. Lee , H. M. Lee , K. Lee , A. Lenon , J. R. Leong , Y. Levin , B. M. Levine , T. G. F. Li , A. Libson , T. B. Littenberg , N. A. Lockerbie , J. Logue , A. L. Lombardi , J. E. Lord , M. Lormand , J. D. Lough , H. Lück , A. P. Lundgren , J. Luo , R. Lynch , Y. Ma , T. MacDonald , B. Machenschalk , M. MacInnis , D. M. Macleod , F. Magana-Sandoval , R. M. Magee , M. Mageswaran , I. Mandel , V. Mandic , V. Mangano , G. L. Mansell , M. Manske , S. Márka , Z. Márka , A. S. Markosyan , E. Maros , I. W. Martin , R. M. Martin , D. V. Martynov , J. N. Marx , K. Mason , T. J. Massinger , M. Masso-Reid , F. Matichard , L. Matone , N. Mavalvala , N. Mazumder , G. Mazzolo , R. McCarthy , D. E. McClelland , S. McCormick , S. C. McGuire , G. McIntyre , J. McIver , D. J. McManus , S. T. McWilliams , G. D. Meadors , A. Melatos , G. Mendell , D. Mendoza-Gandara , R. A. Mercer , E. Merilh , S. Meshkov , C. Messenger , C. Messick , P. M. Meyers , H. Miao , H. Middleton , E. E. Mikhailov , K. N. Mukund , J. Miller , M. Millhouse , J. Ming , S. Mirshekari , C. Mishra , S. Mitra , V. P. Mitrofanov , G. Mitselmakher , R. Mittleman , S. R. P. Mohapatra , B. C. Moore , C. J. Moore , D. Moraru , G. Moreno , S. R. Morriss , K. Mossavi , C. M. Mow-Lowry , C. L. Mueller , G. Mueller , A. W. Muir , Arunava Mukherjee , D. Mukherjee , S. Mukherjee , A. Mullavey , J. Munch , D. J. Murphy , P. G. Murray , A. Mytidis , R. K. Nayak , V. Necula , K. Nedkova , A. Neunzert , G. Newton , T. T. Nguyen , A. B. Nielsen , A. Nitz , D. Nolting , M. E. N. Normandin , L. K. Nuttall , J. Oberling , E. Ochsner , J. O'Dell , E. Oelker , G. H. Ogin , J. J. Oh , S. H. Oh , F. Ohme , M. Oliver , P. Oppermann , Richard J. Oram , B. O'Reilly , R. O'Shaughnessy , C. D. Ott , D. J. Ottaway , R. S. Ottens , H. Overmier , B. J. Owen , A. Pai , S. A. Pai , J. R. Palamos , O. Palashov , A. Pal-Singh , H. Pan , C. Pankow , F. Pannarale , B. C. Pant , M. A. Papa , H. R. Paris , W. Parker , D. Pascucci , Z. Patrick , B. L. Pearlstone , M. Pedraza , L. Pekowsky , A. Pele , S. Penn , R. Pereira , A. Perreca , M. Phelps , V. Pierro , I. M. Pinto , M. Pitkin , A. Post , J. Powell , J. Prasad , V. Predoi , S. S. Premachandra , T. Prestegard , L. R. Price , M. Principe , S. Privitera , R. Prix , L. Prokhorov , O. Puncken , M. Pürrer , H. Qi , J. Qin , V. Quetschke , E. A. Quintero , R. Quitzow-James , F. J. Raab , D. S. Rabeling , H. Radkins , P. Raffai , S. Raja , M. Rakhmanov , V. Raymond , J. Read , C. M. Reed , S. Reid , D. H. Reitze , H. Rew , K. Riles , N. A. Robertson , R. Robie , J. G. Rollins , V. J. Roma , J. D. Romano , G. Romanov , J. H. Romie , S. Rowan , A. Rüdiger , K. Ryan , S. Sachdev , T. Sadecki , L. Sadeghian , M. Saleem , F. Salemi , A. Samajdar , L. Sammut , E. J. Sanchez , V. Sandberg , B. Sandeen , J. R. Sanders , B. S. Sathyaprakash , P. R. Saulson , O. Sauter , R. L. Savage , A. Sawadsky , P. Schale , R. Schilling , J. Schmidt , P. Schmidt , R. Schnabel , R. M. S. Schofield , A. Schönbeck , E. Schreiber , D. Schuette , B. F. Schutz , J. Scott , S. M. Scott , D. Sellers , A. Sergeev , G. Serna , A. Sevigny , D. A. Shaddock , M. S. Shahriar , M. Shaltev , Z. Shao , B. Shapiro , P. Shawhan , A. Sheperd , D. H. Shoemaker , D. M. Shoemaker , X. Siemens , D. Sigg , A. D. Silva , D. Simakov , A. Singer , L. P. Singer , A. Singh , R. Singh , A. M. Sintes , B. J. J. Slagmolen , J. R. Smith , N. D. Smith , R. J. E. Smith , E. J. Son , B. Sorazu , T. Souradeep , A. K. Srivastava , A. Staley , M. Steinke , J. Steinlechner , S. Steinlechner , D. Steinmeyer , B. C. Stephens , R. Stone , K. A. Strain , N. A. Strauss , S. Strigin , R. Sturani , A. L. Stuver , T. Z. Summerscales , L. Sun , P. J. Sutton , M. J. Szczepańczyk , D. Talukder , D. B. Tanner , M. Tápai , S. P. Tarabrin , A. Taracchini , R. Taylor , T. Theeg , M. P. Thirugnanasambandam , E. G. Thomas , M. Thomas , P. Thomas , K. A. Thorne , K. S. Thorne , E. Thrane , V. Tiwari , K. V. Tokmakov , C. Tomlinson , C. V. Torres , C. I. Torrie , D. Töyrä , G. Traylor , D. Trifirò , M. Tse , D. Tuyenbayev , D. Ugolini , C. S. Unnikrishnan , A. L. Urban , S. A. Usman , H. Vahlbruch , G. Vajente , G. Valdes , D. C. Vander-Hyde , A. A. van Veggel , S. Vass , R. Vaulin , A. Vecchio , J. Veitch , P. J. Veitch , K. Venkateswara , S. Vinciguerra , D. J. Vine , S. Vitale , T. Vo , C. Vorvick , W. D. Vousden , S. P. Vyatchanin , A. R. Wade , L. E. Wade , M. Wade , M. Walker , L. Wallace , S. Walsh , H. Wang , M. Wang , X. Wang , Y. Wang , R. L. Ward , J. Warner , B. Weaver , M. Weinert , A. J. Weinstein , R. Weiss , T. Welborn , L. Wen , P. Weßels , T. Westphal , K. Wette , J. T. Whelan , S. E. Whitcomb , D. J. White , B. F. Whiting , R. D. Williams , A. R. Williamson , J. L. Willis , B. Willke , M. H. Wimmer , W. Winkler , C. C. Wipf , H. Wittel , G. Woan , J. Worden , J. L. Wright , G. Wu , J. Yablon , W. Yam , H. Yamamoto , C. C. Yancey , M. J. Yap , H. Yu , M. Zanolin , M. Zevin , F. Zhang , L. Zhang , M. Zhang , Y. Zhang , C. Zhao , M. Zhou , Z. Zhou , X. J. Zhu , M. E. Zucker , S. E. Zuraw , J. Zweizig

An improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors

We improve the accuracy of the effective-one-body (EOB) waveforms that were employed during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing black holes by calibrating them to a set of 141…

广义相对论与量子宇宙学 · 物理学 2017-03-30 Alejandro Bohé , Lijing Shao , Andrea Taracchini , Alessandra Buonanno , Stanislav Babak , Ian W. Harry , Ian Hinder , Serguei Ossokine , Michael Pürrer , Vivien Raymond , Tony Chu , Heather Fong , Prayush Kumar , Harald P. Pfeiffer , Michael Boyle , Daniel A. Hemberger , Lawrence E. Kidder , Geoffrey Lovelace , Mark A. Scheel , Béla Szilágyi

Generating Higher Order Modes from Binary Black Hole mergers with Machine Learning

We introduce a machine learning model designed to rapidly and accurately predict the time domain gravitational wave emission of non-precessing binary black hole coalescences, incorporating the effects of higher order modes of the multipole…

广义相对论与量子宇宙学 · 物理学 2024-04-29 Tim Grimbergen , Stefano Schmidt , Chinmay Kalaghatgi , Chris van den Broeck

Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers

Since the initial detection of Gravitational Waves in 2015, 50 candidate events have been reported by the LIGO-Virgo-KAGRA collaboration. As the current generation of detectors move towards their design sensitivity the rate of these…

广义相对论与量子宇宙学 · 物理学 2022-02-16 Philip Relton , Vivien Raymond

Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers

On 2020 February 24, during their third observing run ("O3"), the Laser Interferometer Gravitational-wave Observatory and Virgo Collaboration (LVC) detected S200224ca: a candidate gravitational wave (GW) event produced by a binary black…

高能天体物理现象 · 物理学 2021-02-10 N. J. Klingler , A. Lien , S. R. Oates , J. A. Kennea , P. A. Evans , A. Tohuvavohu , B. Zhang , K. L. Page , S. B. Cenko , S. D. Barthelmy , A. P. Beardmore , M. G. Bernardini , A. A. Breeveld , P. J. Brown , D. N. Burrows , S. Campana , G. Cusumano , A. D'Aì , P. D'Avanzo , V. D'Elia , M. de Pasquale , S. W. K. Emery , J. Garcia , P. Giommi , C. Gronwall , D. H. Hartmann , H. A. Krimm , N. P. M. Kuin , D. B. Malesani , F. E. Marshall , A. Melandri , J. A. Nousek , P. T. O'Brien , J. P. Osborne , D. M. Palmer , M. J. Page , M. Perri , J. L. Racusin , T. Sakamoto , B. Sbarufatti , J. E. Schlieder , M. H. Siegel , G. Tagliaferri , E. Troja

Eccentric binary black holes: A new framework for numerical relativity waveform surrogates

Mounting evidence indicates that some of the gravitational wave signals observed by the LIGO/Virgo/KAGRA observatories might arise from eccentric compact object binaries, increasing the urgency for accurate waveform models for such systems.…

广义相对论与量子宇宙学 · 物理学 2025-10-03 Peter James Nee , Adhrit Ravichandran , Scott E. Field , Tousif Islam , Harald P. Pfeiffer , Vijay Varma , Michael Boyle , Andrea Ceja , Noora Ghadiri , Lawrence E. Kidder , Prayush Kumar , Akash Maurya , Marlo Morales , Antoni Ramos-Buades , Abhishek Ravishankar , Katie Rink , Hannes R. Rüter , Mark A. Scheel , Md Arif Shaikh , Daniel Tellez

Synergies in analysing binary black hole mergers: Effect of orbital eccentricity, spin-precession, and non-quadrupole modes

A gravitational wave (GW) signal carries imprints of the properties of its source. The ability to extract source properties crucially depends on our prior knowledge of the signal morphology. Even though binary black hole (BBH) mergers are…

广义相对论与量子宇宙学 · 物理学 2024-09-10 Divyajyoti

Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations

Massive black-hole (BH) mergers are predicted to be powerful sources of low-frequency gravitational waves (GWs). Coupling the detection of GWs with an electromagnetic (EM) detection can provide key information about merging BHs and their…

高能天体物理现象 · 物理学 2023-10-03 C. A. Dong-Páez , M. Volonteri , R. S. Beckmann , Y. Dubois , A. Mangiagli , M. Trebitsch , S. Vergani , N. Webb

An eccentric binary black hole inspiral-merger-ringdown gravitational waveform model from numerical relativity and post-Newtonian theory

We present a prescription for computing gravitational waveforms for the inspiral, merger and ringdown of non-spinning eccentric binary black hole systems. The inspiral waveform is computed using the post-Newtonian expansion and the merger…

广义相对论与量子宇宙学 · 物理学 2018-08-15 Ian Hinder , Lawrence E. Kidder , Harald P. Pfeiffer

Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$ rate

Gravitational wave detections are starting to allow us to probe the physical processes in the evolution of very massive stars through the imprints they leave on their final remnants. Stellar evolution theory predicts the existence of a gap…

高能天体物理现象 · 物理学 2020-10-22 Robert Farmer , Mathieu Renzo , Selma de Mink , Maya Fishbach , Stephen Justham

The effect of different eLISA-like configurations on massive black hole parameter estimation

As the theme for the future L3 Cosmic Vision mission, ESA has recently chosen the `Gravitational Wave Universe'. Within this call, a mission concept called eLISA has been proposed. This observatory has a current initial configuration…

广义相对论与量子宇宙学 · 物理学 2015-09-09 Edward K. Porter

The Effects of Resolution on Black Hole Accretion Simulations of Jets

We perform three general-relativistic magnetohydrodynamic simulations of black hole accretion designed to test how sensitive results are to grid resolution in the jet region. The cases differ only in numerics, modelling the same physical…

高能天体物理现象 · 物理学 2020-09-09 Christopher J. White , Fiona Chrystal

Landscape of stellar-mass black-hole spectroscopy with third-generation gravitational-wave detectors

Gravitational-wave black-hole spectroscopy provides a unique opportunity to test the strong-field regime of gravity and the nature of the final object formed in the aftermath of a merger. Here we investigate the prospects for black-hole…

广义相对论与量子宇宙学 · 物理学 2023-09-26 Swetha Bhagwat , Costantino Pacilio , Paolo Pani , Michela Mapelli

Modeling the source of GW150914 with targeted numerical-relativity simulations

In fall of 2015, the two LIGO detectors measured the gravitational wave signal GW150914, which originated from a pair of merging black holes. In the final 0.2 seconds (about 8 gravitational-wave cycles) before the amplitude reached its…

广义相对论与量子宇宙学 · 物理学 2016-11-22 Geoffrey Lovelace , Carlos O. Lousto , James Healy , Mark A. Scheel , Alyssa Garcia , Richard O'Shaughnessy , Michael Boyle , Manuela Campanelli , Daniel A. Hemberger , Lawrence E. Kidder , Harald P. Pfeiffer , Bela Szilagyi , Saul A. Teukolsky , Yosef Zlochower

Forecasting properties of detectable massive binary black hole mergers in the era of space based gravitational-wave detectors

Gravitational waves (GWs) from massive black hole (MBH) mergers will provide a novel way to probe the high-redshift universe and are key to understanding galactic dynamics and evolution. In this work, we analyze MBH mergers, their GW…

高能天体物理现象 · 物理学 2025-11-19 Sourabh Magare , Abhinav Roy , Shasvath J. Kapadia , Nishikanta Khandai , R. Srianand

Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA

We study prospects for detecting extragalactic binary black holes similar to GW150914 by evolved Laser Interferometer Space Antenna (eLISA). We find that the majority of detected binary black holes will not merge within reasonable…

高能天体物理现象 · 物理学 2016-08-30 Koutarou Kyutoku , Naoki Seto

Orbital Evolution of Extreme-Mass-Ratio Black-Hole Binaries with Numerical Relativity

We perform the first fully nonlinear numerical simulations of black-hole binaries with mass ratios 100:1. Our technique for evolving such extreme mass ratios is based on the moving puncture approach with a new gauge condition and an optimal…

广义相对论与量子宇宙学 · 物理学 2011-07-04 Carlos O. Lousto , Yosef Zlochower

Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis

The future space mission LISA will observe a wealth of gravitational-wave sources at millihertz frequencies. Of these, the extreme-mass-ratio inspirals of compact objects into massive black holes are the only sources that combine the…

广义相对论与量子宇宙学 · 物理学 2021-02-08 Alvin J. K. Chua , Michael L. Katz , Niels Warburton , Scott A. Hughes

Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms

Numerical relativity waveforms are a critical resource in the quest to deepen our understanding of the dynamics of, and gravitational waves emitted from, merging binary systems. We present 181 new numerical relativity simulations as the…

广义相对论与量子宇宙学 · 物理学 2025-08-29 Deborah Ferguson , Evelyn Allsup , Surendra Anne , Galina Bouyer , Miguel Gracia-Linares , Hector Iglesias , Aasim Jan , Pablo Laguna , Jacob Lange , Erick Martinez , Filippo Meoni , Ryan Nowicki , Deirdre Shoemaker , Blake Steadham , Max L. Trostel , Bing-Jyun Tsao , Finny Valorz

Are long-term $N$-body simulations reliable?

$N$-body integrations are used to model a wide range of astrophysical dynamics, but they suffer from errors which make their orbits diverge exponentially in time from the correct orbits. Over long time-scales, their reliability needs to be…

地球与行星天体物理 · 物理学 2020-02-26 David M. Hernandez , Sam Hadden , Junichiro Makino