The DOI matches its Crossref record.
Entropy Generation and the Survival of Protogalaxies in an Expanding Universe
Abstract
General formulae are derived for the bulk viscosity, shear viscosity, and heat transport due to radia tion, and for the damping rate of sound waves, in an imperfect relativistic fluid. These results are used to evaluate the cosmological entropy production associated with a nonvanishing mean free time of photons, neutrinos, or gravitons, and to calculate the rate of damping of protogalactic fluctuations in the period immediately prior to the recombination of hydrogen.
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“The quark nuggets evaporate as long as the temperature is above ∼ 50 MeV [99].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [99]
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“It remains to figure out how the CNB entropy could actually be measured: Since the CNB is isotropic, any increase in entropy could only manifest itself macroscopically as an induced dissipative pressure (bulk viscosity [39, 40]).”
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“2 Incidentally, this coefficient for the viscosity was first derived by Masaki (1971), and it differs by a factor of 10 9 from the more com- monly cited value, νa = 4 15 ( E ρc2 ) cλp, in, e.g., Weinberg (1971), Weinberg (1972), and Mihalas & Mihalas (1984).”
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“, for ultrarelativistic and nonrelativistic gases interacting weakly with local forces via binary collisions [3, 4].”
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“It is well known that the adiabatic baryon and photon density perturbations are erased away due to the photon diffusion before and during the recombination epoch (Silk 1968; Sato 1971; Weinberg 1971).”
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“(2.5), we used that, in the very early universe, the damping rate is mainly dominated by the shear viscosity η ( τ ) [8].”
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“…T μν in the fi rst-order gradient expansion is a tiny perturbation that corresponds to all dissipative processes ( heat fl ux, anisotropic stress, and bulk viscosity ) ( Weinberg 1971 ) as where the matrix Δ ij projects to the subspace orthogonal to the fl uid velocity: Δ ij = g ij + u i u j and Π B…”
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“The photon viscosity could also work to transfer angular momentum in a di†erentially rotating, optically thick disk & Laor(Misner 1968 ; Weinberg 1971 ; Masaki 1971 ; Loeb When the efficiency is translated to a-parameter, a D1992). where and are, respectively,p r /(p g ] p r )[L(vr/c)/Lq], pr…”
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“The inclusion of a secondary dilatational/bulk viscosity term à la Weinberg Ṙ/R would be an interesting add-on since our viscous correction is only of the shear type Ṙ/R [26].”
Background
Metadata
- Authors
- Weinberg, S.
- Corresponding author
- Weinberg, Steven
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1971-09
- Volume
- 168
- Pages
- 175
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2006497728
- Cited by
- 734
- References
- 0
- Citations by year
- 2026: 28 · 2025: 21 · 2024: 18 · 2023: 21 · 2022: 18 · 2021: 31 · 2020: 25 · 2019: 12 · 2018: 21 · 2017: 33 · 2016: 30 · 2015: 32 · 2014: 20 · 2013: 31 · 2012: 14
- FWCI
- 8.59
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- The Astrophysical Journal (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- entropy production, protogalaxies, cosmic expansion, bulk viscosity, shear viscosity, radiative heat transport, acoustic damping, mean free time, photon mean free path, neutrino mean free path, hydrogen recombination
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