Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.
Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.
复制标题
观察和定位带有晚期Ligo和晚期处女座的重力波瞬变的前景。
DOI:
10.1007/lrr-2016-1
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发表时间:
2016
影响因子:
40.6
通讯作者:
Zweizig J
中科院分区:
文献类型:
--
作者:
Abbott BP;LIGO Scientific Collaboration;Virgo Collaboration;Abbott R;Abbott TD;Abernathy MR;Acernese F;Ackley K;Adams C;Adams T;Addesso P;Adhikari RX;Adya VB;Affeldt C;Agathos M;Agatsuma K;Aggarwal N;Aguiar OD;Ain A;Ajith P;Allen B;Allocca A;Altin PA;Amariutei DV;Anderson SB;Anderson WG;Arai K;Araya MC;Arceneaux CC;Areeda JS;Arnaud N;Arun KG;Ashton G;Ast M;Aston SM;Astone P;Aufmuth P;Aulbert C;Babak S;Baker PT;Baldaccini F;Ballardin G;Ballmer SW;Barayoga JC;Barclay SE;Barish BC;Barker D;Barone F;Barr B;Barsotti L;Barsuglia M;Barta D;Bartlett J;Bartos I;Bassiri R;Basti A;Batch JC;Baune C;Bavigadda V;Bazzan M;Behnke B;Bejger M;Belczynski C;Bell AS;Bell CJ;Berger BK;Bergman J;Bergmann G;Berry CP;Bersanetti D;Bertolini A;Betzwieser J;Bhagwat S;Bhandare R;Bilenko IA;Billingsley G;Birch J;Birney R;Biscans S;Bisht A;Bitossi M;Biwer C;Bizouard MA;Blackburn JK;Blair CD;Blair D;Blair RM;Bloemen S;Bock O;Bodiya TP;Boer M;Bogaert G;Bogan C;Bohe A;Bojtos P;Bond C;Bondu F;Bonnand R;Bork R;Boschi 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We present a possible observing scenario for the Advanced LIGO and Advanced Virgo 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 determine the expected 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 considered the most promising 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 90% 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 deg2 to 20 deg2 will require at least three detectors of sensitivity within a factor of ∼ 2 of each other and with a broad frequency bandwidth. Should the third LIGO detector be relocated to India as expected, a significant fraction of gravitational-wave signals will be localized to a few square degrees by gravitational-wave observations alone.