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Nucleation of cosmological phase transitions
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“The deflagration front (the bubble wall) moves with the velocity v defl ≪ 1 / √ 3 [90].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [90]
Citations
Cites
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Metadata
- Authors
- Hogan, C. J.
- Affiliations
- California Institute of Technology (US)
- Corresponding author
- Hogan, Craig J.
- ORCID
- Hogan, Craig J.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 1983-12
- Volume
- 133
- Issue
- 3-4
- Pages
- 172-176
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2047506876
- Cited by
- 189
- References
- 18
- Citations by year
- 2026: 7 · 2025: 11 · 2024: 12 · 2023: 4 · 2022: 5 · 2021: 11 · 2020: 14 · 2019: 10 · 2018: 24 · 2017: 7 · 2016: 4 · 2015: 2 · 2014: 2 · 2013: 1 · 2012: 2
- FWCI
- 4.69
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Physics Letters B (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › High-Energy Particle Collisions Research
- Keywords
- cosmological phase transitions, bubble nucleation, first-order phase transition, bubble size, black hole formation, Planck temperature, nucleosynthesis, cosmological inhomogeneities, entropy perturbations, pressure perturbation
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