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

Title:	Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors
Authors:	Abadie J; Abbott BP; Abbott R; Abernathy M; Accadia T; Acerneseac F; Adams C; Adhikari R; Ajith P; Allen B; Allen G; Ceron EA; Amin RS; Anderson SB; Anderson WG; Antonuccia F; Aoudiaa S; Arain MA; Araya M; Aronsson M; Arun KG; Aso Y; Aston S; Astonea P; Atkinson DE; Aufmuth P; Aulbert C; Babak S; Baker P; Ballardin G; Ballmer S; Barker D; Barnum S; Baroneac F; Barr B; Barriga P; Barsotti L; Barsuglia M; Barton MA; Bartos I; Bassiri R; Bastarrika M; Bauchrowitz J; Bauera TS; Behnke B; Beker MG; Benacquista M; Bertolini A; Betzwieser J; Beveridge N; Beyersdorf PT; Bigottaab S; Bilenko IA; Billingsley G; Birch J; Birindellia S; Biswas R; Bitossi M; Bizouard MA; Black E; Blackburn JK; Blackburn L; Blair D; Bland B; Bloma M; Blomberg A; Boccara C; Bock O; Bodiya TP; Bondarescu R; Bondu F; Bonelli L; Bork R; Born M; Bose S; Bosi L; Boyle M; Braccini S; Bradaschia C; Brady PR; Braginsky VB; Brau JE; Breyer J; Bridges DO; Brillet A; Brinkmann M; Brisson V; Britzger M; Brooks AF; Brown DA; Budzynski R; Bulik T; Bulten HJ; Buonanno A; Burguet-Castell J; Burmeister O; Buskulic D; Byer RL; Cadonati L; Cagnoli G; Calloni E; Camp JB; Campagna E; Campsie P; Cannizzo J; Cannon KC; Canuel B; Cao J; Capano C; Carbognani F; Caride S; Caudill S; Cavagli M; Cavalier F; Cavalieri R; Cella G; Cepeda C; Cesarini E; Chalermsongsak T; Chalkley E; Charlton P; Mottin EC; Chelkowski S; Chen Y; Chincarini A; Christensen N; Chua SSY; Chung CTY; Clark D; Clark J; Clayton JH; Cleva F; Coccia E; Colacino CN; Colas J; Colla A; Colombini M; Conte R; Cook D; Corbitt TR; Corda C; Cornish N; Corsi A; Costa CA; Coulon JP; Coward D; Coyne DC; Creighton JDE; Creighton TD; Cruise AM; Culter RM; Cumming A; Cunningham L; Cuoco E; Dahl K; Danilishin SL; Dannenberg R; D'Antonio S; Danzmann K; Dari A; Das K; Dattilo V; Daudert B; Davier M; Davies G; Davis A; Daw EJ; Day R; Dayanga T; De Rosa R; Debra D; Degallaix J; Del Prete M; Dergachev V; DeRosa R; DeSalvo R; Devanka P; Dhurandhar S; Fiore L; Di Lieto A; Di Palma I; Emilio MD; Di Virgilio A; Diaz M; Dietz A; Donovan F; Dooley KL; Doomes EE; Dorsher S; Douglas ESD; Dragocd M; Drever RWP; Driggers JC; Dueck J; Dumas JC; Eberle T; Edgar M; Edwards M; Effler A; Ehrens P; Engel R; Etzel T; Evans M; Evans T; Fafone V; Fairhurst S; Fan Y; Farr BF; Fazi D; Fehrmann H; Feldbaum D; Ferrante I; Fidecaro F; Finn LS; Fiori I; Flaminio R; Flanigan M; Flasch K; Foley S; Forrest C; Forsi E; Fotopoulos N; Fournier JD; Franc J; Frasca S; Frasconi F; Frede M; Frei M; Frei Z; Freise A; Frey R; Fricke TT; Friedrich D; Fritschel P; Frolov VV; Fulda P; Fyffe M; Gammaitoni L; Garofoli JA; Garufiab F; Gemme G; Genin E; Gennai A; Gholami I; Ghosh S; Giaime JA; Giampanis S; Giardina KD; Giazotto A; Gill C; Goetz E; Goggin LM; Gonzalez G; Gorodetsky ML; Gossler S; Gouaty R; Graef C; Granata M; Grant A; Gras S; Gray C; Greenhalgh RJS; Gretarsson AM; Greveriea C; Grosso R; Grote H; Grunewald S; Guidi GM; Gustafson EK; Gustafson R; Hage B; Hall P; Hallam JM; Hammer D; Hammond G; Hanks J; Hanna C; Hanson J; Harms J; Harry GM; Harry IW; Harstad ED; Haughian K; Hayama K; Heefner J; Heitmann H; Hello P; Heng IS; Heptonstall A; Hewitson M; Hild S; Hirose E; Hoak D; Hodge KA; Holt K; Hosken DJ; Hough J; Howell E; Hoyland D; Huet D; Hughey B; Husa S; Huttner SH; Huynh-Dinh T; Ingram DR; Inta R; Isogai T; Ivanov A; Jaranowski P; Johnson WW; Jones DI; Jones G; Jones R; Ju L; Kalmus P; Kalogera V; Kandhasamy S; Kanner J; Katsavounidis E; Kawabe K; Kawamura S; Kawazoe F; Kells W; Keppel DG; Khalaidovski A; Khalili FY; Khazanov EA; Kim C; Kim H; King PJ; Kinzel DL; Kissel JS; Klimenko S; Kondrashov V; Kopparapu R; Koranda S; Kowalska I; Kozak D; Krause T; Kringel V; Krishnamurthy S; Krishnan B; Krolak A; Kuehn G; Kullman J; Kumar R; Kwee P; Landry M; Lang M; Lantz B; Lastzka N; Lazzarini A; Leaci P; Leong J; Leonor I; Leroy N; Letendre N; Li J; Li TGF; Lin H; Lindquist PE; Lockerbie NA; Lodhia D; Lorenzinia M; Lorietteb V; Lormand M; Losurdo G; Lu P; Luan J; Lubinski M; Lucianetti A; Luck H; Lundgren A; Machenschalk B; MacInnis M; Mackowski JM; Mageswaran M; Mailand K; Majoranaa E; Mak C; Man N; Mandel I; Mandic V; Mantovani M; Marchesoni F; Marion F; Marka S; Marka Z; Maros E; Marque J; Martelli F; Martin IW; Martin RM; Marx JN; Mason K; Masserot A; Matichard F; Matone L; Matzner RA; Mavalvala N; McCarthy R; McClelland DE; McGuire SC; McIntyre G; McIvor G; McKechan DJA; Meadors G; Mehmet M; Meier T; Melatos A; Melissinos AC; Mendell G; Menendez DF; Mercer RA; Merill L; Meshkov S; Messenger C; Meyer MS; Miao H; Michel C; Milano L; Miller J; Minenkov Y; Mino Y; Mitra S; Mitrofanov VP; Mitselmakher G; Mittleman R; Moe B; Mohan M; Mohanty SD; Mohapatra SRP; Moraru D; Moreau J; Moreno G; Morgado N; Morgia A; Morioka T; Mors K; Mosca S; Moscatelli V; Mossavi K; Mours B; MowLowry C; Mueller G; Mukherjee S; Mullavey A; Muller-Ebhardt H; Munch J; Murray PG; Nash T; Nawrodt R; Nelson J; Neri I; Newton G; Nishizawa A; Nocera F; Nolting D; Ochsner E; O'Dell J; Ogin GH; Oldenburg RG; O'Reilly B; O'Shaughnessy R; Osthelder C; Ottaway DJ; Ottens RS; Overmier H; Owen BJ; Page A; Pagliaroli G; Palladino L; Palomba C; Pan Y; Pankow C; Paoletti F; Papa MA; Pardi S; Pareja M; Parisi M; Pasqualetti A; Passaquieti R; Passuello D; Patel P; Pedraza M; Pekowsky L; Penn S; Peralta C; Perreca A; Persichetti G; Pichot M; Pickenpack M; Piergiovanni F; Pietkae M; Pinard L; Pinto IM; Pitkin M; Pletsch HJ; Plissi MV; Poggiani R; Postiglione F; Prato M; Predoi V; Price LR; Prijatelj M; Principe M; Privitera S; Prix R; Prodi GA; Prokhorov L; Puncken O; Punturoa M; Puppo P; Quetschke V; Raab FJ; Rabaste O; Rabeling DS; Radke T; Radkins H; Raffai P; Rakhmanov M; Rankins B; Rapagnani P; Raymond V; Re V; Reed CM; Reed T; Regimbau T; Reid S; Reitze DH; Ricci F; Riesen R; Riles K; Roberts P; Robertson NA; Robinet F; Robinson C; Robinson EL; Rocchi A; Roddy S; Rover C; Rogstad S; Rolland L; Rollins J; Romano JD; Romano R; Romie JH; Rosinskag D; Rowan S; Udiger AR; Ruggi P; Ryan K; Sakata S; Sakosky M; Salemi F; Sammut L; de la Jordana LS; Sandberg V; Sannibale V; Santamaria L; Santostasi G; Saraf S; Sassolas B; Sathyaprakash BS; Sato S; Satterthwaite M; Saulson PR; Savage R; Schilling R; Schnabel R; Schofield R; Schulz B; Schutz BF; Schwinberg P; Scott J; Scott SM; Searle AC; Seifert F; Sellers D; Sengupta AS; Sentenac D; Sergeev A; Shaddock DA; Shapiro B; Shawhan P; Shoemaker DH; Sibley A; Siemens X; Sigg D; Singer A; Sintes AM; Skelton G; Slagmolen BJJ; Slutsky J; Smith JR; Smith MR; Smith ND; Somiya K; Sorazu B; Speirits FC; Stein AJ; Stein LC; Steinlechner S; Steplewski S; Stochino A; Stone R; Strain KA; Strigin S; Stroeer A; Sturani R; Stuver AL; Summerscales TZ; Sung M; Susmithan S; Sutton PJ; Swinkels B; Talukder D; Tanner DB; Tarabrin SP; Taylor JR; Taylor R; Thomas P; Thorne KA; Thorne KS; Thrane E; Thuering A; Titsler C; Tokmakov KV; Toncelli A; Tonelli M; Torres C; Torrie CI; Tournefier E; Travasso F; Traylor G; Trias M; Trummer J; Tseng K; Ugolini D; Urbanek K; Vahlbruch H; Vaishnav B; Vajente G; Vallisneri M; van den Branda JFJ; Van den Broeck C; Van der Puttena S; van der Sluys MV; van Veggel AA; Vass S; Vaulin R; Vavoulidis M; Vecchio A; Vedovato G; Veitch J; Veitch PJ; Veltkamp C; Verkindt D; Vetrano F; Vicere A; Villar A; Vineta JY; Vocca H; Vorvick C; Vyachanin SP; Waldman SJ; Wallace L; Wanner A; Ward RL; Wasa M; Wei P; Weinert M; Weinstein AJ; Weiss R; Wen L; Wen S; Wessels P; West M; Westphal T; Wette K; Whelan JT; EWhitcomb S; White DJ; Whiting BF; Wilkinson C; Willems PA; Williams L; Willke B; Winkelmann L; Winkler W; Wipf CC; Wiseman AG; Woan G; Wooley R; Worden J; Yakushin I; Yamamoto H; Yamamoto K; Yeaton-Massey D; Yoshida S; Yu PP; Yvert M; Zanolin M; Zhang L; Zhang Z; Zhao C; Zotov N; Zucker ME; Zweizig J; Belczynski K
Contributors:	Abadie, J; Abbott, Bp; Abbott, R; Abernathy, M; Accadia, T; Acerneseac, F; Adams, C; Adhikari, R; Ajith, P; Allen, B; Allen, G; Ceron, Ea; Amin, R; Anderson, Sb; Anderson, Wg; Antonuccia, F; Aoudiaa, S; Arain, Ma; Araya, M; Aronsson, M; Arun, Kg; Aso, Y; Aston, S; Astonea, P; Atkinson, De; Aufmuth, P; Aulbert, C; Babak, S; Baker, P; Ballardin, G; Ballmer, S; Barker, D; Barnum, S; Baroneac, F; Barr, B; Barriga, P; Barsotti, L; Barsuglia, M; Barton, Ma; Bartos, I; Bassiri, R; Bastarrika, M; Bauchrowitz, J; Bauera, T; Behnke, B; Beker, Mg; Benacquista, M; Bertolini, A; Betzwieser, J; Beveridge, N; Beyersdorf, Pt; Bigottaab, S; Bilenko, Ia; Billingsley, G; Birch, J; Birindellia, S; Biswas, R; Bitossi, M; Bizouard, Ma; Black, E; Blackburn, Jk; Blackburn, L; Blair, D; Bland, B; Bloma, M; Blomberg, A; Boccara, C; Bock, O; Bodiya, Tp; Bondarescu, R; Bondu, F; Bonelli, L; Bork, R; Born, M; Bose, S; Bosi, L; Boyle, M; Braccini, S; Bradaschia, C; Brady, Pr; Braginsky, Vb; Brau, Je; Breyer, J; Bridges, Do; Brillet, A; Brinkmann, M; Brisson, V; Britzger, M; Brooks, Af; Brown, Da; Budzynski, R; Bulik, T; Bulten, Hj; Buonanno, A; Burguet-Castell, J; Burmeister, O; Buskulic, D; Byer, Rl; Cadonati, L; Cagnoli, G
Publication Year:	2010
Collection:	IRIS Università degli Studi di Bologna (CRIS - Current Research Information System)
Subject Terms:	gravitational waves
Description:	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 extrapolations from observed binary pulsars in our galaxy. These yield a likely coalescence rate of 100 Myr−1 per Milky Way Equivalent Galaxy (MWEG), although the rate could plausibly range from 1 Myr−1 MWEG−1 to 1000 Myr−1 MWEG−1 (Kalogera et al 2004 Astrophys. J. 601 L179; Kalogera et al 2004 Astrophys. J. 614 L137 (erratum)). We convert coalescence rates into detection rates based on data from the LIGO S5 and Virgo VSR2 science runs and projected sensitivities for our advanced detectors. Using the detector sensitivities derived from these data, we find a likely detection rate of 0.02 per year for Initial LIGO–Virgo interferometers, with a plausible range between 2 × 10−4 and 0.2 per year. The likely binary neutron–star detection rate for the Advanced LIGO–Virgo network increases to 40 events per year, with a range between 0.4 and 400 per year.
Document Type:	article in journal/newspaper
File Description:	ELETTRONICO
Language:	English
Relation:	info:eu-repo/semantics/altIdentifier/wos/WOS:000280317700001; volume:27; issue:17; firstpage:1; lastpage:20; numberofpages:20; journal:CLASSICAL AND QUANTUM GRAVITY; https://hdl.handle.net/11585/998509
DOI:	10.1088/0264-9381/27/17/173001
Availability:	https://hdl.handle.net/11585/998509; https://doi.org/10.1088/0264-9381/27/17/173001
Accession Number:	edsbas.2DBBCDB5
Database:	BASE