Unifying holographic inflation with holographic dark energy: A covariant approach
In the present paper, we use the holographic approach to describe the early-time acceleration and the late-time acceleration eras of our Universe in a unified manner. Such "holographic unification" is found to have a correspondence with various higher curvature cosmological models with or...
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| Veröffentlicht in: | Physical review. D 2020-07, Vol.102 (2), p.1, Article 023540 |
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| creator | Nojiri, Shin'ichi Odintsov, S. D. Oikonomou, V. K. Paul, Tanmoy |
| description | In the present paper, we use the holographic approach to describe the early-time acceleration and the late-time acceleration eras of our Universe in a unified manner. Such "holographic unification" is found to have a correspondence with various higher curvature cosmological models with or without matter fields. The corresponding holographic cutoffs are determined in terms of the particle horizon and its derivatives, or the future horizon and its derivatives. As a result, the holographic energy density we propose is able to merge various cosmological epochs of the Universe from a holographic point of view. We find the holographic correspondence of several F(R) gravity models, including axion-F(R) gravity models, of several Gauss-Bonnet F(G) models and finally of F(T) models, and in each case we demonstrate that it is possible to describe in a unified way inflation and late-time acceleration in the context of the same holographic model. |
| doi_str_mv | 10.1103/PhysRevD.102.023540 |
| format | Article |
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| source | American Physical Society Journals; Web of Science - Science Citation Index Expanded - 2020<img src="https://exlibris-pub.s3.amazonaws.com/fromwos-v2.jpg" /> |
| subjects | Acceleration Astronomical models Astronomy & Astrophysics Cosmology Dark energy Derivatives Flux density Gravitation Holography Horizon Physical Sciences Physics Physics, Particles & Fields Science & Technology Universe |
| title | Unifying holographic inflation with holographic dark energy: A covariant approach |
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