@article{3df17dd6ed4f4d1c9a644c63a3138237,
title = "Detection prospects of core-collapse supernovae with supernova-optimized third-generation gravitational-wave detectors",
abstract = "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 3×10-27 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.",
author = "Varun Srivastava and Stefan Ballmer and Brown, {Duncan A.} and Chaitanya Afle and Burrows, {Adam S.} and David Radice and David Vartanyan",
note = "Funding Information: We thank Evan Hall and Joshua Smith for their help with GWINC . We thank Geoffrey Lovelace and Christopher Wipf for helpful discussions in regards with the astrophysical implications of the results. V. S., S. B., D. A. B., and C. A. thank the National Science Foundation for support through Grant No. PHY-1836702. A. B., D. R., and D. V. acknowledge support from the U.S. Department of Energy Office of Science and the Office of Advanced Scientific Computing Research via the Scientific Discovery through Advanced Computing (SciDAC4) program and Grant No. DE-SC0018297 (subaward No. 00009650), the U.S. NSF under Grants No. AST-1714267 and No. PHY-1144374, the DOE/ASCR INCITE program under Contract No. DE-AC02-06CH11357, a Blue Waters PRAC (under Grants No. OCI-0725070, No. OAC-1809073, and No. ACI-1238993), and the National Energy Research Scientific Computing Center (NERSC) under Contract No. DE-AC03-76SF00098. D. A. B. acknowledges NSF Grant No. PHY-1748958 to the Kavli Institute for Theoretical Physics for support. Publisher Copyright: {\textcopyright} 2019 American Physical Society.",
year = "2019",
month = aug,
day = "23",
doi = "10.1103/PhysRevD.100.043026",
language = "English (US)",
volume = "100",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "4",
}