The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Gravitational waves from first-order cosmological phase transitions
Abstract
A first-order cosmological phase transition that proceeds through the nucleation and collision of true-vacuum bubbles is a potent source of gravitational radiation. Possibilities for such include first-order inflation, grand-unified-theory-symmetry breaking, and electroweak-symmetry breaking. We have calculated gravity-wave production from the collision of two scalar-field vacuum bubbles, and, using an approximation based upon these results, from the collision of 20 to 30 vacuum bubbles. We present estimates of the relic background of gravitational waves produced by a first-order phase transition; in general, ${\mathrm{\ensuremath{\Omega}}}_{\mathrm{GW}}$\ensuremath{\sim}${10}^{\mathrm{\ensuremath{-}}9}$ and f\ensuremath{\sim}(${10}^{\mathrm{\ensuremath{-}}6}$ Hz) (T/1 GeV).
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Citations
Cites
Witten, E. (1984) · Physical Review D · doi:10.1103/physrevd.30.272 · Cited by 3,452
Nucleation of cosmological phase transitions
Hogan, C. J. (1983) · Physics Letters B · doi:10.1016/0370-2693(83)90553-1 · Cited by 189
Cited by
Piscopo, M. L., Spannowsky, M., & Waite, P. (2019) · Physical Review D · doi:10.1103/physrevd.100.016002 · Cited by 117
Metadata
- Authors
- Kosowsky, A., Turner, M. S., & Watkins, R.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1992-10-05
- Volume
- 69
- Issue
- 14
- Pages
- 2026-2029
- ISSN
- 0031-9007 (ISSN-L)
- OpenAlex
- W2060583654
- Cited by
- 507
- References
- 2
- FWCI
- 6.55
- Type
- journal article
- Language
- en
- Open access
- closed
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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