Cosmological baryon diffusion and nucleosynthesis
Abstract
The diffusion rate of baryons through the big-bang plasma is calculated. Fluctuations in baryon density in the early Universe lead to inhomogeneities in the neutron-proton ratio, due to the differential diffusion of these particles through the radiation plasma. For certain types of nonlinear fluctuations, some nucleosynthesis would occur in very neutron-rich regions. Nuclear products of homogeneous neutron-enriched regions are evaluated numerically using a standard reaction network and these results are used to estimate final abundances in an inhomogeneous universe. Net deuterium and lithium abundances tend to increase and the net helium abundance tends to decrease compared to an unperturbed standard model. It is suggested that pronounced nonlinear baryon-density fluctuations produced in QCD- or electroweak-epoch phase transitions could alter abundances sufficiently to make a closed baryonic universe consistent with current observations of these elements. In such a model the abundance of heavier elements (C,N,O, etc.) increases significantly and approaches observable levels. Abundances can be used to place constraints on extreme scenarios for phase transitions at these epochs.
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If the QCD transition is strong enough, these clumps could be detected by gravitational femtolensing.
“If the QCD transition is strong enough, these clumps could be detected by gravitational femtolensing [108].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [108]
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Stochastic Isocurvature Baryon Fluctuations, Baryon Diffusion, and Primordial Nucleosynthesis
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Big-bang nucleosynthesis and the quark-hadron phase transition
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Random Spherical Hyperbolic Diffusion
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The number of neutrino species
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Baryon density contrast and strangeness abundance during the big bang confinement phase transition
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Zero-metallicity stellar sources and the reionization epoch
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“…very high baryon density in a small fraction of the universe and in these regions some fraction of heavy elements were already synthesized during primordial nucleosynthesis (Applegate et al. 1987); (Thomas et al. 1994); (Jedamzik et al. 1994); (Kurki-Suonio et al. 1977); (Jedamzik & Rehm 2001).”
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Measurement of the H2 (n,γ) H3 reaction cross section between 10 and 550 keV
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- Authors
- Applegate, J. H., Hogan, C. J., & Scherrer, R. J.
- Affiliations
- Columbia University (US)
- University of Arizona (US)
- University of Chicago (US)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1987-02-15
- Volume
- 35
- Issue
- 4
- Pages
- 1151-1160
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2034982956
- Cited by
- 246
- References
- 24
- Citations by year
- 2026: 6 · 2025: 1 · 2024: 2 · 2022: 3 · 2021: 3 · 2020: 2 · 2019: 5 · 2018: 3 · 2017: 4 · 2016: 2 · 2015: 1 · 2014: 1 · 2013: 2 · 2012: 1
- FWCI
- 41.07
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- PubMed (publishedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Nuclear physics research studies
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Keywords
- big bang nucleosynthesis, baryon density fluctuations, neutron-to-proton ratio, deuterium abundance, lithium abundance, helium abundance, phase transitions, QCD phase transition, electroweak phase transition, closed universe, primordial abundances, reaction networks
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