Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

@article{Collaboration2010PredictionsFT,
  title={Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors},
  author={Ligo Scientific Collaboration and Virgo Collaboration J. Abadie and Brad Abbott and Richard J. Abbott and Matthew Robert Abernathy and T. Accadia and Fausto Acernese and Carl Adams and R X Adhikari and Parameswaran Ajith and Bruce Allen and Gabrielle Allen and E. Amador Ceron and Rupal S. Amin and Stuart B. Anderson and Warren G. Anderson and F. Antonucci and S. Aoudia and Muzammil A. Arain and M. C. Araya and Marcus Aronsson and K. G. Arun and Yoichi Aso and Stuart M. Aston and Pia Astone and D. E. Atkinson and Peter Aufmuth and Carsten Aulbert and Stanislav Babak and Paul T. Baker and Giulio Ballardin and Stefan W. Ballmer and Daniel H. N. Barker and Samuel Barnum and Fabrizio Barone and B. W. Barr and Pablo Jos{\'e} Barriga and Lisa Barsotti and Matteo Barsuglia and Mark Andrew Barton and Imre Bartos and Riccardo Bassiri and M. Bastarrika and J{\"o}ran Bauchrowitz and Th. S. Bauer and Beate Behnke and M. G. Beker and Matthew J. Benacquista and Alessandro Bertolini and Joe Betzwieser and Nicole Beveridge and P. T. Beyersdorf and Stefano Bigotta and I. A. Bilenko and G Billingsley and Jeremy Birch and S. Birindelli and Rahul Biswas and Massimiliano Bitossi and M. A. Bizouard and Eric D. Black and J. K. Blackburn and Lindy Blackburn and David G Blair and B. Bland and M. Blom and Adam Blomberg and Claude A. Boccara and Oliver Bock and T. P. Bodiya and Ruxandra Bondarescu and F. Bondu and L. Bonelli and R. G. Bork and Michael Born and Suvadeep Bose and L. Bosi and Michael Boyle and Saverio Braccini and C. Bradaschia and Patrick R. Brady and Vladimir B. Braginsky and James E. Brau and J. Breyer and D. O. Bridges and A. Brillet and Martin Brinkmann and V. Brisson and Michael Britzger and A. F. Brooks and D. A. Brown and R. Budzy'nski and Tomasz Bulik and H. J. Bulten and Alessandra Buonanno and Jordi Burguet-Castell and Oliver Burmeister and D. Buskulic and Robert L. Byer and Laura Cadonati and Gianpietro Cagnoli and Enrico Calloni and Jordan B. Camp and E. Campagna and Paul Campsie and John K. Cannizzo and Kipp C. Cannon and Benjamin Canuel and J. Cao and C. D. Capano and Franco Carbognani and Santiago Caride and Sarah Caudill and Marco Cavagli{\`a} and F. Cavalier and R. Cavalieri and Giancarlo Cella and Carlos Cepeda and Elisa Cesarini and Tara Chalermsongsak and E. Chalkley and Philip R. Charlton and {\'E}ric Chassande-Mottin and Simon Chelkowski and Y. R. Chen and Andrea Chincarini and Nelson Christensen and Sheon S Y Chua and C. T. Y. Chung and Donald E. Clark and J A Clark and J. H. Clayton and F. Cleva and Eugenio Coccia and C. N. Colacino and Jacques Colas and Alberto Colla and Maria Perla Colombini and Roberto Conte and D. Cook and Thomas R. Corbitt and Christian Corda and Neil J. Cornish and Alessandra Corsi and C. A. Costa and J.-P. Coulon and D. M. Coward and D. C. Coyne and Jolien D. E. Creighton and Teviet Creighton and Adrian Michael Cruise and R. M. Culter and Andrew Cumming and L. Cunningham and Elena Cuoco and Katrin Dahl and S L Danilishin and Robert Dannenberg and Sabrina D’Antonio and Karsten Danzmann and Anna Dari and K. Das and Vincenzino Dattilo and Britta Daudert and M. Davier and G. S. Cabourn Davies and A. Davis and E. J. Daw and Richard N. Day and Thilina Dayanga and Rosario De Rosa and Daniel B. DeBra and J{\'e}r{\^o}me Degallaix and M. del Prete and Vladimir Dergachev and R. T. Derosa and Riccardo DeSalvo and P. Devanka and Sanjeev V. Dhurandhar and L. Di Fiore and Alberto Di Lieto and I. Di Palma and Maurizio Di Paolo Emilio and Angela Di Virgilio and M. C. D'iaz and Alexander Dietz and Frederick J. Donovan and K L Dooley and E. E. Doomes and Steven Dorsher and Ewan S. Douglas and M. Drago and Ronald W. P. Drever and J C Driggers and J. Dueck and J-C. Dumas and Tobias Eberle and Matthew P. Edgar and Matthew C. Edwards and Anamaria Effler and Phil Ehrens and Ralph Engel and Taylor M. Etzel and Matthew Evans and Timothy Evans and V Fafone and Stephen Fairhurst and Y. Fan and Benjamin Farr and Diego Fazi and Henning Fehrmann and David M. Feldbaum and I. Ferrante and Francesco Fidecaro and Lee Samuel Finn and Irene Fiori and R. Flaminio and M. C. Flanigan and Kurt Flasch and Stephany Foley and C. Forrest and Ericka Forsi and Nickolas V Fotopoulos and J.-D. Fournier and Janyce Franc and Sergio Frasca and F. Frasconi and Maik Frede and Melissa A. Frei and Zsolt Frei and Andreas Freise and Raymond E. Frey and T. T. Fricke and Daniel Friedrich and P. Fritschel and Valery Victor Frolov and P. J. Fulda and Matthew Fyffe and Luca Gammaitoni and Justin Garofoli and F. Garufi and Gianluca Gemme and Emmanuelle G{\'e}nin and A. Gennai and Iraj Gholami and S. Ghosh and Joseph A. Giaime and Stefanos Giampanis and K. D. Giardina and A. Giazotto and C. Gill and E Goetz and Lisa M. Goggin and Gabriela Gonz'alez and Mikhail L. Gorodetsky and Stefan Gossler and R. Gouaty and Christian Graef and Massimo Granata and A. Grant and Slawomir Gras and C. Gray and R. Justin S. Greenhalgh and A M Gretarsson and Caroline Greverie and Ryan Grosso and Hartmut Grote and S. Grunewald and G. Guidi and Eric K. Gustafson and Richard Gustafson and Boris Hage and Peter Hall and J. M. Hallam and David Hammer and Giles D. Hammond and Jonathan Hanks and Chad Hanna and James E. Hanson and Jan Harms and Gregory M. Harry and I. W. Harry and E. D. Harstad and K. Haughian and Kazuhiro Hayama and J. W. Heefner and H. Heitmann and P. Hello and Ik Siong Heng and Alastair Heptonstall and Martin Hewitson and Stefan Hild and Eiichi Hirose and David Hoak and Kari Alison Hodge and K. Holt and D. J. Hosken and James Hough and E J Howell and David Hoyland and Dominique Huet and Barbara J. Hughey and Sascha Husa and S. H. Huttner and T. Huynh--Dinh and D. R. Ingram and Ra Inta and Tomoki Isogai and Anton B. Ivanov and Piotr Jaranowski and W. W. Johnson and D. I. Jones and G. Jones and R. W. L. Jones and Li Ju and Peter Kalmus and Vassiliki Kalogera and Shivaraj Kandhasamy and Jonah B. Kanner and Erotokritos Katsavounidis and Keita Kawabe and Seiji Kawamura and Fumiko Kawazoe and William P. Kells and Drew Garvin Keppel and Alexander Khalaidovski and Farid Ya. Khalili and E. A. Khazanov and C. Kim and H. Kim and P. J. King and D. L. Kinzel and J. S. Kissel and Sergey Klimenko and V. T. Kondrashov and Ravi kumar Kopparapu and Scott Koranda and Izabela Jonek Kowalska and Darby Kozak and T. Krause and V. Kringel and Suraj Krishnamurthy and Badri Krishnan and Andrzej Kr'olak and G. Kuehn and J. M. Kullman and R. Kumar and Patrick Kwee and Michael Landry and M. M. Lang and Brian Lantz and Nico Lastzka and Albert Lazzarini and Paola Leaci and Jonathan Leong and Isabel B. Leonor and Nicolas Leroy and Nicolas Letendre and J. Li and T. G. F. Li and H. L. Lin and P. E. Lindquist and N. A. Lockerbie and Deepali Lodhia and Marco Lorenzini and Vincent Loriette and Marc Lormand and Giovanni Losurdo and P. Lu and Jing Luan and M. J. Lubinski and Antonio Lucianetti and Harald Luck and Andrew Lundgren and Bernd Machenschalk and Myron Macinnis and J.-M. Mackowski and M. Mageswaran and K. Mailand and E. Majorana and C. Mak and Na Man and Ilya Mandel and Vuk Mandic and Maddalena Mantovani and Fabio Marchesoni and F. Marion and Szabolcs M'arka and Zsuzsa M'arka and Edward Maros and J. Marque and F. Martelli and Iain W. Martin and R. M. Martin and J. N. Marx and K. O. Mason and A. Masserot and F. Matichard and Luca Matone and Richard A. Matzner and Nergis Mavalvala and Robert McCarthy and D. E. McClelland and Scott C. McGuire and G. McIntyre and G. McIvor and David McKechan and Grant David Meadors and Moritz Mehmet and Torsten Meier and Andrew Melatos and Adrian C. Melissinos and Greg Mendell and D. F. Men'endez and R. A. Mercer and L. Merill and Sydney Meshkov and Chris Messenger and Manuel Meyer and Haixing Miao and Christophe Michel and Leopoldo Milano and J. R. Miller and Yury Minenkov and Yasushi Mino and Subhasish Mitra and Vp. Mitrofanov and Gena Mitselmakher and Richard K Mittleman and Brian Moe and M. Mohan and Soumya D. Mohanty and Satyanarayan Ray Pitambar Mohapatra and Daniel Moraru and Jacques Moreau and Gerardo Moreno and N. Morgado and A. Morgia and Tomoko Morioka and K. Mors and Simona Mosca and Vincenzo B. Moscatelli and Kasem Mossavi and B. Mours and C Mowlowry and Guido Mueller and Suvodip Mukherjee and Adam J Mullavey and Helge Muller-Ebhardt and Jesper Munch and P. G. Murray and Thomas Nash and Ronny Nawrodt and Janice Nelson and Igor Neri and G. P. Newton and Atsushi J. Nishizawa and F. Nocera and Dan Nolting and Evan Ochsner and Joseph O'Dell and G. H. Ogin and R. G. Oldenburg and Brian O'reilly and Richard O’Shaughnessy and Charles Osthelder and David J. Ottaway and R. S. Ottens and Harry Overmier and Benjamin James Owen and Amanda J. Page and G. Pagliaroli and Luigi Palladino and Cristiano Palomba and Y. B. Pan and Christopher Pankow and Federico Paoletti and Maria Alessandra Papa and Silvio Pardi and M. J. Pareja and Maria Parisi and A. Pasqualetti and R. Passaquieti and D. Passuello and P. Patel and M. Pedraza and Larne Pekowsky and Stephen Penn and Carlos Peralta and Antonio Perreca and Gianluca Persichetti and Mikhael Pichot and M. Pickenpack and Francesco Piergiovanni and Maciej Pietka and L. Pinard and Innocenzo M. Pinto and Matthew Pitkin and H. J. Pletsch and Michael V Plissi and R. Poggiani and Fabio Postiglione and Mirko Prato and Valeriu Predoi and Larry R. Price and Mirko Prijatelj and M. Principe and S. Privitera and Reinhard Prix and Giovanni Andrea Prodi and Leonid Prokhorov and Oliver Puncken and M. Punturo and P. Puppo and Volker Quetschke and F. J. Raab and Olivier Rabaste and D. S. Rabeling and Thomas Radke and Hugh Radkins and Peter Raffai and Malik Rakhmanov and Brooke Rankins and P. Rapagnani and V Raymond and Virginia Re and C. M. Reed and T. Reed and Tania Regimbau and Stuart Reid and D. H. Reitze and F. Ricci and R. Riesen and Keith Riles and P. Roberts and N. A. Robertson and Florent Robinet and C. A. K. Robinson and E. L. Robinson and Alessandro Rocchi and Shaun Roddy and Christian Rover and S. Rogstad and Lo{\"i}c Rolland and Jameson Graef Rollins and J. D. Romano and Rocco Romano and Janeen H. Romie and D. Rosi'nska and Sheila Rowan and A. Rudiger and P. Ruggi and Kris Ryan and Shihori Sakata and M. Sakosky and Francesco Salemi and Letizia Sammut and Ls de la Jordana and V. D. Sandberg and Virginio Sannibale and Luc'ia Santamar'ia and Giovanni Santostasi and Siddhant Saraf and Beno{\^i}t Sassolas and Bangalore Sathyaprakash and S. Sato and Mark Satterthwaite and Peter Saulson and Richard L. Savage and Roland Schilling and Roman Schnabel and Robert M. S. Schofield and Bernhard Schulz and Bernard F. Schutz and P. B. Schwinberg and J. Scott and Susan M. Scott and Antony C. Searle and Frank Seifert and Danny Sellers and Anand S. Sengupta and Daniel Sentenac and A. S. Sergeev and Daniel A. Shaddock and B. Shapiro and Peter Shawhan and D. H. Shoemaker and Anna Sibley and Xavier Siemens and Daniel Sigg and Andrej Singer and Alicia M. Sintes and G. R. Skelton and B. J. J. Slagmolen and Jacob Slutsky and J. R. Smith and Madison R Smith and Nicolas de Mateo Smith and Kentaro Somiya and Borja Sorazu and Fiona C. Speirits and Andrew J. Stein and Leo C. Stein and Sebastian Steinlechner and S. Steplewski and Alberto Stochino and Robert Stone and Kenneth Strain and Sergey Strigin and Alexander Stroeer and Riccardo Sturani and Amber L. Stuver and Tiffany Summerscales and Myungkee Sung and Sunil Susmithan and P. Sutton and Bas Swinkels and Dipongkar Talukder and David B. Tanner and S. P. Tarabrin and J. R. Taylor and R. D. Taylor and Pieter Thomas and Keith A. Thorne and Kip S. Thorne and Eric Thrane and Ann Thuring and C. Titsler and K. Tokmakov and Alessandra Toncelli and Mauro Tonelli and Cristina Torres and Calum I. Torrie and E. Tournefier and Flavio Travasso and Gary Traylor and Miquel Trias and Jonas Trummer and K. Tseng and Dennis Wayne Ugolini and Karel E. Urbanek and Henning Vahlbruch and B. Vaishnav and Gabriele Vajente and Michele Vallisneri and J. F. J. van den Brand and Chris van den Broeck and S. van. der. Putten and M. van der Sluys and A. A. van Veggel and Steve Vass and Ruslan Vaulin and Miltiadis Vavoulidis and Alberto Vecchio and Gabriele Vedovato and John Veitch and Peter J. Veitch and Christian Veltkamp and D. Verkindt and F. Vetrano and Andrea Vicer'e and Akira E. Villar and J.-Y. Vinet and Helios Vocca and Cheryl Vorvick and S. P. Vyachanin and Samuel J. Waldman and L. Wallace and Alexander Wanner and Robert L. Ward and Michal Was and P. Wei and Michael Weinert and Allan J. Weinstein and Rainer Weiss and Longping Wen and S. Wen and Peter Wessels and M. West and Tobias Westphal and Karl Wette and John T. Whelan and S. E. Whitcomb and Darren J. White and Bernard Whiting and Clive R. Wilkinson and Phil A. Willems and L. Williams and Benno Willke and Lutz Winkelmann and Walter Winkler and Christopher C. Wipf and A. G. Wiseman and Graham Woan and R. Wooley and John R. Worden and Igor Yakushin and H. Yamamoto and K. Yamamoto and David Yeaton-Massey and Sanichiro Yoshida and P. P. Yu and M. Yvert and Michele Zanolin and L. Zhang and Z. Zhang and C. Zhao and Natalia V. Zotov and Michael Edward Zucker and J. G. Zweizig and Krzysztof Belczyński},
  journal={Classical and Quantum Gravity},
  year={2010},
  volume={27},
  pages={173001-173001}
}
We present an up-to-date, comprehensive summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo. Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters and are still uncertain. The most confident among these estimates are the rate predictions for coalescing binary neutron stars which are based on… 
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References

SHOWING 1-10 OF 118 REFERENCES
THE COSMIC COALESCENCE RATES FOR DOUBLE NEUTRON STAR BINARIES
We report on the newly increased event rates due to the recent discovery of the highly relativistic binary pulsar J07373039. Using a rigorous statistical method, we present the calculations reported
Host Galaxies Catalog Used in LIGO Searches for Compact Binary Coalescence Events
An up-to-date catalog of nearby galaxies considered to be hosts of binary compact objects is provided, with complete information about sky position, distance, extinction-corrected blue luminosity,
The Probability Distribution of Binary Pulsar Coalescence Rates. I. Double Neutron Star Systems in the Galactic Field
Estimates of the Galactic coalescence rate () of close binaries with two neutron stars (NS-NS) are known to be uncertain by large factors (about 2 orders of magnitude) mainly because of the small
The Probability Distribution of Binary Pulsar Coalescence Rates
Inspiraling binary systems are good candidates for being detected by ground‐based gravitational‐wave detectors. In this work, we present a statistical analysis method to estimate the coalescence rate
The Rate of Neutron Star Binary Mergers in the Universe: Minimal Predictions for Gravity Wave Detectors
Of the many sources which gravitational wave observatories might see, merging neutron star binaries are the most predictable. Their waveforms at the observable frequencies are easy to calculate. And
Galactic distribution of merging neutron stars and black holes – prospects for short gamma-ray burst progenitors and LIGO/VIRGO
We have performed a detailed population synthesis on a large number (2 x 10 7 ) of binary systems in order to investigate the properties of massive double degenerate binaries. We have included new
Impact of star formation inhomogeneities on merger rates and interpretation of LIGO results
Within the next decade, ground based gravitational-wave detectors are in principle capable of determining the compact object merger rate per unit volume of the local universe to better than 20% with
The Coalescence Rate of Double Neutron Star Systems
We estimate the coalescence rate of close binaries with two neutron stars (NS) and discuss the prospects for the detection of NS-NS inspiral events by ground-based gravitational-wave observatories,
The Probability Distribution of the Double Neutron Star Coalescence Rate and Predictions for More Detections
We present an analysis method that allows us to estimate the Galactic formation of radio pulsar populations based on their observed properties and our understanding of survey selection effects. More
Short γ-ray bursts and gravitational waves from dynamically formed merging binaries
Merging binary systems consisting of two collapsed objects are among the most promising sources of high frequency gravitational wave, GW, signals for ground based interferometers. Double neutron star
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