Supercooling, entropy production, and bubble kinetics in the quark-hadron phase transition in the early universe
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The detailed analysis in ref.[91] leads to the conclusion that the picture of homogeneous bubble nucleation, where bubbles form from statistical fluctuations, is false for the most probable cosmological scenarios.
“The detailed analysis in ref.[91] leads to the conclusion that the picture of homogeneous bubble nucleation, where bubbles form from statistical fluctuations, is false for the most probable cosmological scenarios.”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [91]
If Δ_rms T > 5 × 10^-5, it is quite likely that the condition for d_nuc > λ_smooth is met.
“If ∆ rms T > 5 × 10 -5 , it is quite likely that this condition is met.”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [91]
For the scale-invariant spectrum (n_s = 1), the rms temperature fluctuation at the QCD scale is ∆_rms T(k_QCD) ≈ 2 × 10^-5.
“For the scale-invariant spectrum ( n s = 1) it is found[91] ∆ rms T ( k QCD ) ≈ 2 × 10 -5 .”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [91]
At the QCD transition neutrinos travel freely on scales λ_ν-mfp ≈ 10^-6 R_H, and fluctuations on the diffusion scale of neutrinos are washed out by the time of the QCD transition.
“This study revealed that at the QCD transition neutrinos travel freely on scales λ ν -mfp ≈ 10 -6 R H , and that fluctuations on the diffusion scale of neutrinos are washed out by the time of the QCD transition:”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [91]
A new scenario for the cosmological QCD transition was developed in ref.[91] in which a small scale cut-off in the spectrum of primordial temperature fluctuations from collisional damping by neutrinos is included.
“A new scenario for the cosmological QCD transition was developed in ref.[91] in which a small scale cut-off in the spectrum of primordial temperature fluctuations from collisional damping by neutrinos [92, 93] is included.”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [91]
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Rezzolla, L., & Zanotti, O. (2013) · Oxford University Press eBooks · doi:10.1093/acprof:oso/9780198528906.003.0006
Numerical Relativistic Hydrodynamics: High-Order Methods
Rezzolla, L., & Zanotti, O. (2013) · Oxford University Press eBooks · doi:10.1093/acprof:oso/9780198528906.003.0010
Kim, J. E. (2020) · Corfu Summer Institute School and Workshops on Elementary Particle Physics and Gravity (CORFU) · doi:10.22323/1.376.0151
- Authors
- DeGrand, T., & Kajantie, K.
- Affiliations
- University of Helsinki (FI)
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 1984-11
- Volume
- 147
- Issue
- 4-5
- Pages
- 273-278
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2015544831
- Cited by
- 109
- References
- 20
- Citations by year
- 2026: 1 · 2023: 2 · 2022: 2 · 2020: 2 · 2019: 5 · 2018: 3 · 2014: 2 · 2013: 21 · 2012: 2
- FWCI
- 6.69
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Physics Letters B (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › High-Energy Particle Collisions Research
- 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
- Keywords
- supercooling, quark-hadron phase transition, entropy production, bubble growth, neutrino diffusion, early universe, critical temperature, energy density
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