The DOI matches its Crossref record; 7 of the 7 references it cites were found in a registry or an index.
Origin of the matter-antimatter asymmetry
Open accessAbstract
Although the origin of matter-antimatter asymmetry remains unknown, continuing advances in theory and improved experimental limits have ruled out some scenarios for baryogenesis, for example, sphaleron baryogenesis at the electroweak phase transition in the Standard Model. At the same time, the success of cosmological inflation and the prospects for discovering supersymmetry at the Large Hadron Collider have put some other models in sharper focus. We review the current state of our understanding of baryogenesis with emphasis on those scenarios that we consider most plausible.
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Citations
Cites
Inflationary universe: A possible solution to the horizon and flatness problems
Guth, A. H. (1981) · Physical Review D · doi:10.1103/physrevd.23.347 · Cited by 9,983
Linde, A. D. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)91219-9 · Cited by 6,405
Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
Albrecht, A., & Steinhardt, P. J. (1982) · Physical Review Letters · doi:10.1103/physrevlett.48.1220 · Cited by 4,981
Barygenesis without grand unification
Fukugita, M., & Yanagida, T. (1986) · Physics Letters B · doi:10.1016/0370-2693(86)91126-3 · Cited by 3,879
Symmetry Breaking through Bell-Jackiw Anomalies
't Hooft, G. (1976) · Physical Review Letters · doi:10.1103/physrevlett.37.8 · Cited by 3,362
On anomalous electroweak baryon-number non-conservation in the early universe
Kuzmin, V. A., Rubakov, V. A., & Shaposhnikov, M. E. (1985) · Physics Letters B · doi:10.1016/0370-2693(85)91028-7 · Cited by 3,008 · cited 3×
“This is called electroweak baryogenesis (Kuzmin, Rubakov, and Shaposhnikov, 1985).”
BackgroundCsikor, F., Fodor, Z., Hegedüs, P., Jakovác, A., Katz, S. D., & Piróth, A. (2000) · Physical Review Letters · doi:10.1103/physrevlett.85.932 · Cited by 30 · cited 1×
“Then two-loop effects (Espinosa, 1996; Bodeker et al., 1997) change the scalar potential sufficiently to allow for a first-order phase transition; lattice simulations support this perturbative result (Laine and Rummukainen, 1998; Csikor et al., 2000).”
Background
Cited by
The degree of fine-tuning in our universe — and others
Adams, F. C. (2019) · Physics Reports · doi:10.1016/j.physrep.2019.02.001 · Cited by 62
A Fortunate Universe: Life in a Finely Tuned Cosmos
(2016) · Thammasat University Digital Collections · doi:10.1017/9781316661413 · Cited by 48
Neukart, F. (2025) · Entropy · doi:10.3390/e27020103 · Cited by 4
Metadata
- Authors
- Dine, M., & Kusenko, A.
- Venue
- Reviews of Modern Physics
- Publisher
- American Physical Society (APS)
- Published
- 2003-12-16
- Volume
- 76
- Issue
- 1
- Pages
- 1-30
- ISSN
- 0034-6861 (ISSN-L)
- 1539-0756
- OpenAlex
- W2139830614
- Cited by
- 667
- References
- 7
- FWCI
- 12.04
- Type
- journal article
- Language
- en
- Open access
- green
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