Gravity assisted dark energy dominance and cosmic acceleration
By Shin'ichi Nojiri, Sergei D. Odintsov. 2004
314 citations recorded by the source corpus.
Abstract It is proposed that dark energy may become dominant over standard matter due to universe expansion (curvature decrease). Two models: non-linear gravity–matter system and modified gravity may provide an effective phantom or effective quintessence dark energy which complies with the conjecture. The effective quintessence naturally describes current cosmic speed-up.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/cc99b7c2a0cd4eb7ac7d06fb8f0c8489cb0ef709
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In Astronomy and Astrophysics
- Francisco S. N. Lobo
- Tiberiu Harko
- T. Sotiriou
- Valerio Faraoni
- Salvatore Capozziello
- S. Tsujikawa
- Sergei D. Odintsov
- Shin'ichi Nojiri
In Nuclear and High Energy Physics
- Tiberiu Harko
- Francisco S. N. Lobo
- Valerio Faraoni
- T. Sotiriou
- Salvatore Capozziello
- S. Tsujikawa
- Sergei D. Odintsov
- Shin'ichi Nojiri
Citations in the corpus
- Generalized Curvature-Matter Couplings in Modified Gravity (2014, background): “The specific cases of a curvature coupling to dark energy [10–12], the Maxwell field [13] and an explicit curvature-Yang–Mills coupling [14] was also explored in the context of inflation and of the late-time cosmic acceleration.”
- Imperfect Dark Energy from Kinetic Gravity Braiding (2010, unknown): “recent works [40, 41, 42, 43, 44], contrary to [45, 46].”