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Title: Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run

Journal Article · · Physical Review Letters

We place constraints on the normalized energy density in gravitational waves from first-order strong phase transitions using data from Advanced LIGO and Virgo’s first, second, and third observing runs. First, adopting a broken power law model, we place 95% confidence level upper limits simultaneously on the gravitational-wave energy density at 25 Hz from unresolved compact binary mergers, ΩCBC < 6.1 × 10–9, and strong first-order phase transitions, ΩBPL < 4.4 × 10–9. The inclusion of the former is necessary since we expect this astrophysical signal to be the foreground of any detected spectrum. We then consider two more complex phenomenological models, limiting at 25 Hz the gravitational-wave background due to bubble collisions to Ωpt < 5.0 × 10–9 and the background due to sound waves to Ωpt < 5.8 × 10–9 at 95% confidence level for phase transitions occurring at temperatures above 108 GeV.

Research Organization:
Univ. of Oklahoma, Norman, OK (United States); Univ. of Utah, Salt Lake City, UT (United States)
Sponsoring Organization:
USDOE Office of Science (SC); National Science Foundation (NSF); Ministry of Economic Affairs and Digital Transformation of Spain (MINECO); Science and Technology Facilities Council (STFC) (United Kingdom)
Grant/Contract Number:
SC0009956; SC0009959; PHY-0757058; PHY-0823459; SEV-2016- 0588; PGC2018-101858-B-I00; ST/P000258/1
OSTI ID:
1777661
Alternate ID(s):
OSTI ID: 1851229
Journal Information:
Physical Review Letters, Journal Name: Physical Review Letters Vol. 126 Journal Issue: 15; ISSN 0031-9007
Publisher:
American Physical SocietyCopyright Statement
Country of Publication:
United States
Language:
English

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