A dark energy quintessence model of the universe
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Publication:5217702
DOI10.1142/S0217732320500029zbMath1431.83190arXiv1905.10801OpenAlexW2946598268MaRDI QIDQ5217702
Anirudh Pradhan, Aroonkumar Beesham, Gopi Kant Goswami
Publication date: 26 February 2020
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1905.10801
Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Dark matter and dark energy (83C56)
Cites Work
- An interacting and non-interacting two-fluid dark energy models in FRW universe with time dependent deceleration parameter
- Bianchi V cosmology with a specific Hubble parameter
- Thermodynamics and two-fluid cosmological models
- Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation
- Acceleration of the universe with a simple trigonometric potential
- Exact scalar field cosmologies
- DYNAMICS OF DARK ENERGY
- Two-fluid cosmological models
- Cosmological Inflation and Large-Scale Structure
- Scenario of two-fluid dark energy models in Bianchi type-III Universe
- Transit cosmological models in FRW universe under the two-fluid scenario
- Transit dark energy string cosmological models with perfect fluid in F(R,T)-gravity
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