Ricci–Gauss–Bonnet holographic dark energy in Chern–Simons modified gravity: A flat FLRW quintessence-dominated universe
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Publication:5218284
DOI10.1142/S0217732320500078zbMath1431.83122arXiv1901.04849WikidataQ127091323 ScholiaQ127091323MaRDI QIDQ5218284
Publication date: 2 March 2020
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1901.04849
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)
Related Items (3)
Note on dark energy and cosmic transit in a scale-invariance cosmology ⋮ The Rényi holographic dark energy model in Chern–Simons gravity: Some cosmological implications ⋮ Some cosmological features of 4D Gauss–Bonnet gravity with varying cosmological constant
Cites Work
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- From Inflation to Dark Energy in the Non-Minimal Modified Gravity
- Topological origin of holographic principle: Application to wormholes
- Exact solutions for scalar field cosmology in f(R) gravity
- An alternative to quintessence
- Quintessence model with double exponential potential
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