This dataset contains the compact binary populations that were used in the Cosmic Explorer MPSAC White paper1 (submitted to the NSF MPSAC ngGW Subcommittee) and the accompanying technical paper2. Contents: 1. 1-year populations for binary black hole (BBH), binary neutron star (BNS), neutron star-black hole (NSBH), intermediate mass binary black hole (IMBBH), Population III (Pop 3) binary black holes and primordial black hole (PBH) mergers. It also contains the SNRs and measurement errors on intrinsic and extrinsic parameters calculated using gwbench3. 2. 1/4-year sub-population of BNS mergers for which errors on tidal parameters were calculated. 3. An ipython notebook (instructions.ipynb) that shows how the data can be used. References: 1. Evans, Matthew et al. Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee (2023). arXiv: 2306.13745 [gr-qc]. 2. Gupta, Ish et al. Characterizing Gravitational Wave Detector Networks: From A# to Cosmic Explorer (2023). In preparation. 3. Borhanian, Ssohrab. GWBENCH: a novel Fisher information package for gravitational-wave benchmarking. Class. Quant. Grav. 38, 175014 (2021). arXiv: 2010.15202 [gr-qc].
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Achieving a cosmological reach: from Advanced LIGO to the next generation of terrestrial gravitational wave detectors
Following a decade of unprecedented success through LIGO and Virgo’s observations of compact binary coalescences, gravitational wave astronomy is now recognized as a key tool in our continued efforts to understand the Universe and our place within it. Far from resting on their laurels though, the gravitational wave community is forging ahead with major plans for the future. The proposed “ultimate terrestrial gravitational wave detector facility” Cosmic Explorer recently received a boost with significant funding from the NSF to proceed with a conceptual design. This paper surveys the current state-of-the-art ground-based gravitational wave detector facilities, and their planned near-term upgrades. After motivating the next-generation Cosmic Explorer concept with a discussion of the key science targets, this paper describes some of the unique technical challenges it faces, including a focus on the ongoing optical design of Cosmic Explorer’s 40 km-scale laser interferometers.
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- PAR ID:
- 10526188
- Editor(s):
- de_Groot, Peter J; Picart, Pascal; Guzman, Felipe
- Publisher / Repository:
- SPIE
- Date Published:
- ISBN:
- 9781510673120
- Page Range / eLocation ID:
- 28
- Format(s):
- Medium: X
- Location:
- Strasbourg, France
- Sponsoring Org:
- National Science Foundation
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