Tsallis holographic dark energy model with event horizon cutoff in modified gravity
arXiv:2208.13320 · doi:10.1142/S0219887822502346
Abstract
We considered the Tsallis holographic dark energy model in frames of Nojiri-Odintsov gravity with . For IR cutoff event horizon is taken. The cosmological evolution of such universe is investigated for various initial conditions and values of parameters. The dependence of the Hubble parameter from time in the future has an oscillations. It is shown that for appearance of singularities are typical and the time up to these singularities can be relatively small from cosmological viewpoint. The singularity is associated with the zero of second deribative of on . It is interesting to note that these models can describe observational data from Ia supernovae astrophysics and dependence of the Hubble parameter from redshift at least not worse than canonical CDM model.
arXiv comment20 pp., 7 figures; to appear in Int. J. Geom. Meth. Mod. Phys
References in corpus (40)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Extended Theories of Gravity
- Cosmological Constant - the Weight of the Vacuum
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- Dark Energy and the Accelerating Universe
- A Model of Holographic Dark Energy
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Constraints on the redshift dependence of the dark energy potential
- A 6% measurement of the Hubble parameter at : direct evidence of the epoch of cosmic re-acceleration
- Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
- Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z2
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Baryon Acoustic Oscillations in the Lyα forest of BOSS DR11 quasars
- Palatini Approach to Modified Gravity: f(R) Theories and Beyond
- Black hole thermodynamical entropy
- Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
- Quasar-Lyman Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations
- The Physics of Cosmic Acceleration
- Holographic Dark Energy
- The Holographic Dark Energy in a Non-flat Universe
- Approaches to Understanding Cosmic Acceleration
- Tsallis Holographic Dark Energy
- Dark Matter and Collider Phenomenology of Universal Extra Dimensions
- Generalized entropy formalism and a new holographic dark energy model
- Black holes, cosmological solutions, future singularities, and their thermodynamical properties in modified gravity theories
- Supernova Constraints on a holographic dark energy model
- Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics
- Covariant Generalized Holographic Dark Energy and Accelerating Universe
- Modified cosmology from extended entropy with varying exponent
- Tsallis holographic dark energy in the Brans-Dicke cosmology
- A Note on Tsallis Holographic Dark Energy
- gravity and Tsallis holographic dark energy
- Some models of holographic dark energy on the Randall-Sundrum brane and observational data