Inflation from tsunami-waves
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The standard model of particle physics has the main ingredients for baryogenesis.
“Notably, the standard model of particle physics has the main ingredients for baryogenesis[45, 48]:”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [45]
The Introduction (p. 1) discusses particle-physics-motivated models of inflation, and the Conclusions (p. 25) describe inflation driven by a quantum state. Neither passage addresses whether the standard model has the main ingredients for baryogenesis; searches for “baryogenesis” and the claimed standard-model connection found no relevant passage in our copy. (LLM, conf=0.76)
Experimental — accuracy not yet measuredThere is a large body of observational evidence that suggests there is more matter than antimatter in the Universe up to scales of the order of the Hubble radius.
“There is a large body of observational evidence that suggests that the there is more matter than antimatter in the Universe up to scales of the order of the Hubble radius[44, 45].”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [45]
The Introduction (p. 1) discusses observational evidence from cosmic microwave background anisotropies for inflation, not evidence of a matter–antimatter imbalance. Searches for matter versus antimatter, baryon asymmetry, and the Hubble-radius scale found no passage in our copy addressing the attributed claim. (LLM, conf=0.76)
Experimental — accuracy not yet measuredThe second term proportional to φ^3 in the one-loop effective potential arises from the gauge field contribution and is responsible for a first order phase transition.
“The second term proportional to ϕ 3 arises from the gauge field contribution and is responsible for a first order phase transition.”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [45]
The Introduction (p. 2) and Section 2 (p. 4) describe a scalar-inflaton model, while Section 3.1.2 (pp. 16–17) discusses its effective classical potential. Searches for a gauge-field contribution, a cubic term in a one-loop effective potential, and a first-order phase transition found no passage in our copy addressing the claim; some formulas are not decoded. (LLM, conf=0.76)
Experimental — accuracy not yet measured
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Self-citation
Flagged first, then by citations
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Sorted by citations
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Self-citationThe δ N formula is the dynamical renormalization group
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The δN formula is the dynamical renormalization group
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Quantum inflaton, primordial perturbations, and CMB fluctuations
Cao, F. J., de Vega, H. J., & Sanchez, N. G. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.70.083528 · Cited by 15 · see citing works
Self-citationCao, F. J., de Vega, H. J., & Sanchez, N. G. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.083508 · Cited by 12 · see citing works
Self-citationBoyanovsky, D., de Vega, H. J., & Sanchez, N. G. (2005) · Nuclear Physics B - Proceedings Supplements · doi:10.1016/j.nuclphysbps.2005.04.055 · Cited by 3 · see citing works
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Self-citationBoyanovsky, D., de Vega, H. J., & Sanchez, N. G. (2005) · Cited by 3 · see citing works
Self-citationNoise-induced phase transitions in field-dependent relaxational dynamics: The Gaussian ansatz
Cao, F. J., Wood, K. B., & Lindenberg, K. (2007) · Physical Review E · doi:10.1103/physreve.76.051111 · Cited by 2 · see citing works
Self-citationQuantum inflaton, primordial metric perturbations and CMB fluctuations
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Self-citationInitial States and Time Evolution in Nonequilibrium Quantum Field Theory
Álvarez-Estrada, R. F. (2007) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2006.11.062
Early Cosmology and Fundamental PhysicsPreprint
de Vega, H. J. (2003) · arXiv (Cornell University)
Early Cosmology and Fundamental PhysicsPreprint
de Vega, H. J. (2003) · arXiv (Cornell University) · doi:10.48550/arxiv.astro-ph/0307477
Early Cosmology and Fundamental Physics
de Vega, H. J. (2003) · Springer eBooks · doi:10.1007/978-94-007-1058-0_1
- Authors
- Boyanovsky, D., Cao, F. J., & de Vega, H. J.
- Affiliations
- University of Pittsburgh (US)
- Laboratoire de Physique Théorique et Hautes Energies (FR)
- Venue
- Nuclear Physics B
- Publisher
- Elsevier BV
- Published
- 2002-06
- Volume
- 632
- Issue
- 1-3
- Pages
- 121-154
- ISSN
- 0550-3213 (ISSN-L)
- OpenAlex
- W2094290175
- Cited by
- 23
- References
- 32
- Citations by year
- 2013: 2
- FWCI
- 2.54
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Nuclear Physics B (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- cosmic inflation, tsunami waves, quantum condensates, chaotic inflation, slow-roll inflation, scale factor evolution, scalar perturbations, power spectrum
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