Detection prospects of core-collapse supernovae with supernova-optimized third-generation gravitational-wave detectors

被引:37
作者
Srivastava, Varun [1 ]
Ballmer, Stefan [1 ]
Brown, Duncan A. [1 ]
Afle, Chaitan A. [1 ]
Burrows, Adam [2 ]
Radice, David [2 ,3 ]
Vartanyan, David [2 ]
机构
[1] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA
[2] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[3] Inst Adv Study, 1 Einstein Dr, Princeton, NJ 08540 USA
基金
美国国家科学基金会;
关键词
SIMULATIONS; NEUTRINO; SIGNALS; EMISSION; SEARCH; RATES;
D O I
10.1103/PhysRevD.100.043026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss how to optimize the third-generation gravitational-wave detector to maximize the range to detect core-collapse supernovae. Based on three-dimensional simulations for core-collapse and the corresponding gravitational-wave waveform emitted, the corresponding detection range for these waveforms is limited to within our Galaxy even in the era of third-generation detectors. The corresponding event rate is two per century. We find from the waveforms that to detect core-collapse supernovae with an event rate of one per year, the gravitational-wave detectors need a strain sensitivity of 3 x 10(-27) Hz(-1/2) in a frequency range from 100 to 1500 Hz. We also explore detector configurations technologically beyond the scope of third-generation detectors. We find with these improvements, the event rate for gravitational-wave observations from core-collapse supernovae is still low, but is improved to one in twenty years.
引用
收藏
页数:12
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