Holographic dark energy models in higher derivative torsion corrected modified teleparallel gravity
DOI10.1142/S0219887818500676zbMath1386.83141OpenAlexW2771293444MaRDI QIDQ4609896
Publication date: 26 March 2018
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0219887818500676
cosmological parametersphantom divide lineholographic dark energy modelshigher order torsion corrected modified teleparallel gravity
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Determinants and determinant bundles, analytic torsion (58J52) Astrophysical cosmology (85A40)
Cites Work
- Unnamed Item
- Cosmology of \(F(T)\) gravity and k-essence
- Interacting modified holographic dark energy in Kaluza-Klein universe
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Validity of the generalized second law of thermodynamics of the universe bounded by the event horizon in holographic dark energy model
- Energy conditions in generalized teleparallel gravity models
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Gravitational scalar–tensor theory
- Phase space analysis in a model of f(T) gravity with nonlinear sign changeable interactions
- On the expanding phase of a singular bounce and intermediate inflation: The modified gravity description
- The generalized second law of gravitational thermodynamics on the apparent and event horizons in FRW cosmology
- Pilgrim dark energy
- Thermodynamics of interacting holographic dark energy with the apparent horizon as an IR cutoff
- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- GRAVITATIONAL CHERENKOV RADIATION FROM EXTENDED THEORIES OF GRAVITY
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Scalar field reconstruction of power-law entropy-corrected holographic dark energy
- LOCALLY ROTATIONALLY SYMMETRIC BIANCHI TYPE-I COSMOLOGICAL MODEL IN f(T) GRAVITY: FROM EARLY TO DARK ENERGY DOMINATED UNIVERSE
- Interacting holographic dark energy
- An alternative to quintessence
- Reconstruction and deceleration-acceleration transitions in modified gravity
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