Astrophysical science metrics for next-generation gravitational-wave detectors

被引:33
|
作者
Adhikari, R. X. [1 ]
Ajith, P. [2 ]
Chen, Y. [3 ]
Clark, J. A. [4 ]
Dergachev, V [5 ]
Fotopoulos, N., V [1 ]
Gossan, S. E. [1 ]
Mandel, I [6 ,7 ,8 ,9 ]
Okounkova, M. [3 ]
Raymond, V [10 ]
Read, J. S. [11 ]
机构
[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
[2] Tata Inst Fundamental Res, Int Ctr Theoret Sci, Bangalore 560089, Karnataka, India
[3] CALTECH, TAPIR, Pasadena, CA 91125 USA
[4] Georgia Tech, Atlanta, GA USA
[5] Max Planck Inst Gravitat Phys, Callinstr 38, D-30167 Hannover, Germany
[6] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England
[7] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[8] Monash Univ, Monash Ctr Astrophys, Sch Phys & Astron, Clayton, Vic 3800, Australia
[9] Australian Res Council Ctr Excellence Gravitat Wa, OzGrav, Hawthorn, Vic, Australia
[10] Cardiff Univ, Cardiff Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales
[11] Calif State Univ Fullerton, Fullerton, CA 92634 USA
基金
美国国家科学基金会;
关键词
gravitational waves; black holes; gravitational-wave detectors; EQUATION-OF-STATE; GAMMA-RAY BURSTS; MAGNETIZED NEUTRON-STARS; CORE-COLLAPSE; BLACK-HOLES; COMPACT-OBJECT; POPULATION SYNTHESIS; GIANT FLARE; AXISYMMETRICAL SIMULATIONS; BINARY;
D O I
10.1088/1361-6382/ab3cff
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The second generation of gravitational-wave (GW) detectors are being built and tuned all over the world. The detection of signals from binary black holes is beginning to fulfil the promise of GW astronomy. In this work, we examine several possible configurations for third-generation laser interferometers in existing km-scale facilities. We propose a set of astrophysically motivated metrics to evaluate detector performance. We measure the impact of detector design choices against these metrics, providing a quantitative cost-benefit analyses of the resulting scientific payoffs.
引用
收藏
页数:36
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