Non-interacting Barrow-holographic dark energy in FRW-universe with quintessence behavior
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Publication:6140853
DOI10.1142/S0219887823501396MaRDI QIDQ6140853
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Publication date: 22 January 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Dark matter and dark energy (83C56)
Cites Work
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- An interacting and non-interacting two-fluid dark energy models in FRW universe with time dependent deceleration parameter
- Interacting holographic dark energy model in non-flat universe
- The area of a rough black hole
- Can modified gravity explain accelerated cosmic expansion?
- Generalized Chaplygin gas model: dark energy -- dark matter unification and CMBR con\-straints
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Modified Friedmann equations from Tsallis entropy
- Barrow entropic dark energy: a member of generalized holographic dark energy family
- Big bang nucleosynthesis constraints on Barrow entropy
- Holographic inflation
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Holographic dark energy
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Acceleration of the universe with a simple trigonometric potential
- The holographic principle
- DYNAMICS OF DARK ENERGY
- THE COSMOLOGICAL DYNAMICS OF INTERACTING HOLOGRAPHIC DARK ENERGY MODEL
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Cosmological parameters from SDSS and WMAP
- Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
- CURVATURE QUINTESSENCE
- The world as a hologram
- Barrow Entropy Cosmology: an observational approach with a hint of stability analysis
- Modified cosmology through spacetime thermodynamics and Barrow horizon entropy
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Probable Values of the Cosmological Constant in a Holographic Theory
- Black Holes and Entropy
- THE MINIMAL CURVATURE OF THE UNIVERSE IN MODIFIED GRAVITY AND CONFORMAL ANOMALY RESOLUTION OF THE INSTABILITIES
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