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Formalizing the slow-roll approximation in inflation
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The meaning of the inflationary slow-roll approximation is formalized. Comparisons are made between an approach based on the Hamilton-Jacobi equations, governing the evolution of the Hubble parameter, and the usual scenario based on the evolution of the potential energy density. The vital role of the inflationary attractor solution is emphasized, and some of its properties described. We propose a new measure of inflation, based upon contraction of the comoving Hubble length as opposed to the usual e-foldings of physical expansion, and derive relevant formulas. We introduce an infinite hierarchy of slow-roll parameters, and show that only a finite number of them are required to produce results to a given order. The extension of the slow-roll approximation into an analytic slow-roll expansion, converging on the exact solution, is provided. Its role in calculations of inflationary dynamics is discussed. We explore rational approximants as a method of extending the range of convergence of the slow-roll expansion up to, and beyond, the end of inflation.
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“The agreement between the WMAP results[15, 16, 17, 18] and the most recent analysis of the primordial deuterium abundance[46] yields”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [46]
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Martin, J., Ringeval, C., & Trotta, R. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.063524 · Cited by 88
Attractor behavior of phantom cosmology
Guo, Z., Yun-song Piao, A., & Zhang, Y. (2004) · Physics Letters B · doi:10.1016/j.physletb.2004.05.048 · Cited by 82
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Metadata
- Authors
- Liddle, A. R., Parsons, P., & Barrow, J. D.
- Affiliations
- University of Sussex (GB)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1994-12-15
- Volume
- 50
- Issue
- 12
- Pages
- 7222-7232
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2067502036
- Cited by
- 714
- References
- 21
- Citations by year
- 2026: 28 · 2025: 40 · 2024: 48 · 2023: 34 · 2022: 33 · 2021: 30 · 2020: 41 · 2019: 36 · 2018: 39 · 2017: 45 · 2016: 35 · 2015: 39 · 2014: 19 · 2013: 16 · 2012: 15
- FWCI
- 11.74
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (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 › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- slow-roll approximation, cosmic inflation, Hamilton-Jacobi equation, Hubble parameter evolution, inflationary attractors, slow-roll parameters, rational approximants, end of inflation, scalar field potential
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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