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MODIFIED GRAVITATIONAL THEORIES AND COSMIC ACCELERATION
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Modified gravitational theories can provide alternatives to dark energy as an explaination for the observed late-time cosmic acceleration. Several examples of low-curvature corrections to the Einstein-Hilbert action are studied. These models generically contain unstable de Sitter solutions and, depending on the parameters of the theory, can exhibit late time accelerating attractor solutions.
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Some models built from more general invariants than the Ricci scalar were shown to exhibit late-time self-accelerating expansion without a dark energy component.
“A revived interest was raised into them in the early 2000s as some models were shown to exhibit late-time self-accelerating expansion without a dark energy component (Carroll et al. 2005; Easson 2004; Easson et al. 2005).”
From Testing general relativity in cosmology (2019) · cites this paper as Easson 2004
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“The FLRW solutions of theories with powers of R, RμνR and RμνρσR μνρσ added to the Einstein-Hilbert action were also studied in [455], where the possibility of late-time accelerating expansion was considered.”
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“…Carloni et al., 2008a; Carloni and Dunsby, 2007; Carloni et al., 2005, 2007; Carroll et al., 2005; Clifton, 2006a, 2007; Clifton and Barrow, 2005b; Easson, 2004; Fay et al., 2007a,b; Goheer et al., 2007, 2008; Leach et al., 2006, 2007; Li and Barrow, 2007; Nojiri and Odintsov, 2004b; Sami et al.,…”
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“Originally the model f(R) = R − α/R (α > 0, n > 0) was proposed to explain the late-time cosmic acceleration [113, 120, 114, 143] (see also [456, 559, 17, 223, 212, 16, 137, 62] for related works).”
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Metadata
- Authors
- EASSON, D. A.
- Affiliations
- Syracuse University (US)
- Corresponding author
- EASSON, DAMIEN A.
- ORCID
- EASSON, DAMIEN A.
- Venue
- International Journal of Modern Physics A
- Publisher
- World Scientific Pub Co Pte Lt
- Published
- 2004-12-20
- Volume
- 19
- Issue
- 31
- Pages
- 5343-5350
- ISSN
- 0217-751X (ISSN-L)
- 1793-656X
- OpenAlex
- W1889600657
- Cited by
- 124
- References
- 1
- Citations by year
- 2026: 1 · 2025: 5 · 2024: 6 · 2023: 3 · 2022: 3 · 2021: 4 · 2019: 2 · 2018: 2 · 2017: 5 · 2016: 5 · 2015: 3 · 2014: 4 · 2013: 1 · 2012: 4
- FWCI
- 7.86
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- International Journal of Modern Physics A (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
- modified gravity, dark energy alternatives, late-time cosmic acceleration, Einstein-Hilbert action, de Sitter instability, cosmological constant
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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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