Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

利用高级LIGO、高级Virgo和KAGRA观测和定位引力波瞬变信号的前景

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作者：Abbott,B P,Abbott,R,Abbott,T D,Abernathy,M R,Acernese,F,Ackley,K,Adams,C,Adams,T,Addesso,P,Adhikari,R X,Adya,V B,Affeldt,C,Agathos,M,Agatsuma,K,Aggarwal,N,Aguiar,O D,Aiello,L,Ain,A,Ajith,P,Akutsu,T,Allen,B,Allocca,A,Altin,P A,Ananyeva,A,Anderson,S B,Anderson,W G,Ando,M,Appert,S,Arai,K,Araya,A,Araya,M C,Areeda,J S,Arnaud,N,Arun,K G,Asada,H,Ascenzi,S,Ashton,G,Aso,Y,Ast,M,Aston,S M,Astone,P,Atsuta,S,Aufmuth,P,Aulbert,C,Avila-Alvarez,A,Awai,K,Babak,S,Bacon,P,Bader,M K M,Baiotti,L,Baker,P T,Baldaccini,F,Ballardin,G,Ballmer,S W,Barayoga,J C,Barclay,S E,Barish,B C,Barker,D,Barone,F,Barr,B,Barsotti,L,Barsuglia,M,Barta,D,Bartlett,J,Barton,M A,Bartos,I,Bassiri,R,Basti,A,Batch,J C,Baune,C,Bavigadda,V,Bazzan,M,Bécsy,B,Beer,C,Bejger,M,Belahcene,I,Belgin,M,Bell,A S,Berger,B K,Bergmann,G,Berry,C P L,Bersanetti,D,Bertolini,A,Betzwieser,J,Bhagwat,S,Bhandare,R,Bilenko,I A,Billingsley,G,Billman,C R,Birch,J,Birney,R,Birnholtz,O,Biscans,S,Bisht,A,Bitossi,M,Biwer,C,Bizouard,M A,Blackburn,J K,Blackman,J,Blair,C D,Blair,D G,Blair,R M,Bloemen,S,Bock,O,Boer,M,Bogaert,G,Bohe,A,Bondu,F,Bonnand,R,Boom,B A,Bork,R,Boschi,V,Bose,S,Bouffanais,Y,Bozzi,A,Bradaschia,C,Brady,P R,Braginsky,V B,Branchesi,M,Brau,J E,Briant,T,Brillet,A,Brinkmann,M,Brisson,V,Brockill,P,Broida,J E,Brooks,A F,Brown,D A,Brown,D D,Brown,N M,Brunett,S,Buchanan,C C,Buikema,A,Bulik,T,Bulten,H J,Buonanno,A,Buskulic,D,Buy,C,Byer,R L,Cabero,M,Cadonati,L,Cagnoli,G,Cahillane,C,Calderón Bustillo,J,Callister,T A,Calloni,E,Camp,J B,Cannon,K C,Cao,H,Cao,J,Capano,C D,Capocasa,E,Carbognani,F,Caride,S,Casanueva Diaz,J,Casentini,C,Caudill,S,Cavaglià,M,Cavalier,F,Cavalieri,R,Cella,G,Cepeda,C B,Cerboni Baiardi,L,Cerretani,G,Cesarini,E,Chamberlin,S J,Chan,M,Chao,S,Charlton,P,Chassande-Mottin,E,Cheeseboro,B D,Chen,H Y,Chen,Y,Cheng,H-P,Chincarini,A,Chiummo,A,Chmiel,T,Cho,H S,Cho,M,Chow,J H,Christensen,N,Chu,Q,Chua,A J K,Chua,S,Chung,S,Ciani,G,Clara,F,Clark,J A,Cleva,F,Cocchieri,C,Coccia,E,Cohadon,P-F,Colla,A,Collette,C G,Cominsky,L,Constancio,M Jr,Conti,L,Cooper,S J,Corbitt,T R,Cornish,N,Corsi,A,Cortese,S,Costa,C A,Coughlin,M W,Coughlin,S B,Coulon,J-P,Countryman,S T,Couvares,P,Covas,P B,Cowan,E E,Coward,D M,Cowart,M J,Coyne,D C,Coyne,R,Creighton,J D E,Creighton,T D,Cripe,J,Crowder,S G,Cullen,T J,Cumming,A,Cunningham,L,Cuoco,E,Canton,T Dal,Danilishin,S L,D'Antonio,S,Danzmann,K,Dasgupta,A,Da Silva Costa,C F,Dattilo,V,Dave,I,Davier,M,Davies,G S,Davis,D,Daw,E J,Day,B,Day,R,De,S,DeBra,D,Debreczeni,G,Degallaix,J,De Laurentis,M,Deléglise,S,Del Pozzo,W,Denker,T,Dent,T,Dergachev,V,De Rosa,R,DeRosa,R T,DeSalvo,R,Devine,R C,Dhurandhar,S,Díaz,M C,Fiore,L Di,Giovanni,M Di,Girolamo,T Di,Lieto,A Di,Pace,S Di,Palma,I Di,Virgilio,A Di,Doctor,Z,Doi,K,Dolique,V,Donovan,F,Dooley,K L,Doravari,S,Dorrington,I,Douglas,R,Dovale Álvarez,M,Downes,T P,Drago,M,Drever,R W P,Driggers,J C,Du,Z,Ducrot,M,Dwyer,S E,Eda,K,Edo,T B,Edwards,M C,Effler,A,Eggenstein,H-B,Ehrens,P,Eichholz,J,Eikenberry,S S,Eisenstein,R A,Essick,R 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A,Kijbunchoo,N,Kim,C,Kim,H,Kim,J C,Kim,J,Kim,W,Kim,Y-M,Kimbrell,S J,Kimura,N,King,E J,King,P J,Kirchhoff,R,Kissel,J S,Klein,B,Kleybolte,L,Klimenko,S,Koch,P,Koehlenbeck,S M,Kojima,Y,Kokeyama,K,Koley,S,Komori,K,Kondrashov,V,Kontos,A,Korobko,M,Korth,W Z,Kotake,K,Kowalska,I,Kozak,D B,Krämer,C,Kringel,V,Krishnan,B,Królak,A,Kuehn,G,Kumar,P,Kumar,Rahul,Kumar,Rakesh,Kuo,L,Kuroda,K,Kutynia,A,Kuwahara,Y,Lackey,B D,Landry,M,Lang,R N,Lange,J,Lantz,B,Lanza,R K,Lartaux-Vollard,A,Lasky,P D,Laxen,M,Lazzarini,A,Lazzaro,C,Leaci,P,Leavey,S,Lebigot,E O,Lee,C H,Lee,H K,Lee,H M,Lee,H W,Lee,K,Lehmann,J,Lenon,A,Leonardi,M,Leong,J R,Leroy,N,Letendre,N,Levin,Y,Li,T G F,Libson,A,Littenberg,T B,Liu,J,Lockerbie,N A,Lombardi,A L,London,L T,Lord,J E,Lorenzini,M,Loriette,V,Lormand,M,Losurdo,G,Lough,J D,Lousto,C O,Lovelace,G,Lück,H,Lundgren,A P,Lynch,R,Ma,Y,Macfoy,S,Machenschalk,B,MacInnis,M,Macleod,D M,Magaña-Sandoval,F,Majorana,E,Maksimovic,I,Malvezzi,V,Man,N,Mandic,V,Mangano,V,Mano,S,Mansell,G 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期刊：Living Reviews in Relativity影响因子：62.500
时间：2018起止号：2018;21(1):3
doi：10.1007/s41114-018-0012-9研究方向： 信号转导

Abstract

We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger astronomy with gravitational waves. We estimate the sensitivity of the network to transient gravitational-wave signals, and study the capability of the network to determine the sky location of the source. We report our findings for gravitational-wave transients, with particular focus on gravitational-wave signals from the inspiral of binary neutron star systems, which are the most promising targets for multi-messenger astronomy. The ability to localize the sources of the detected signals depends on the geographical distribution of the detectors and their relative sensitivity, and [Formula: see text] credible regions can be as large as thousands of square degrees when only two sensitive detectors are operational. Determining the sky position of a significant fraction of detected signals to areas of 5-[Formula: see text] requires at least three detectors of sensitivity within a factor of [Formula: see text] of each other and with a broad frequency bandwidth. When all detectors, including KAGRA and the third LIGO detector in India, reach design sensitivity, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.

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