Observational constraints on Tsallis holographic dark energy with Ricci horizon cutoff

Abstract

In this research, we are interested in constraining the nonlinear interacting and noninteracting Tsallis holographic dark energy (THDE) with Ricci horizon cutoff by employing three observational datasets. To this aim, the THDE with Ricci horizon considering the noninteraction and nonlinear interaction terms will be fitted by the SNe Ia, SNe Ia+H(z), and SNe Ia+H(z)+GRB samples to investigate the Hubble ($H(z)$), dark energy equation of state (${\omega }_{DE}$), effective equation of state (${\omega }_{eff}$), and deceleration ($q$) parameters. Investigating the $H(z)$ parameter illustrates that our models are in good consistent with respect to observation. Also, it can reveal the turning point for both noninteracting and nonlinear interacting THDE with Ricci cutoff in the late time era. Next, the analysis of the ${\omega }_{DE}$ for our models displays that the dark energy can experience the phantom state at the current time. However, it lies in the quintessence regime in the early era and approaches the cosmological constant in the late-time epoch. Similar results will be for the ${\omega }_{eff}$ parameter with this difference that the ${\omega }_{eff}$ will experience the quintessence region at the current redshift. Next to the mentioned parameters, the study of the $q$ parameter indicates that the models satisfy an acceptable transition phase from the matter to the dark energy-dominated era. After that, the classical stability ($v_s^2$) will be analyzed for our models. The $v_s^2$ shows that the noninteracting and nonlinear interacting THDE with Ricci cutoff will be stable in the past era, unstable in the present, and progressive epochs. Then, we will employ the $Jerk$ ($J$) and $OM$ parameters to distinguish between our models and the $\Lambda CDM$ model. Finally, we will calculate the age of the Universe for the THDE and nonlinear interacting THDE with Ricci as the IR cutoff.

arXiv comment35 pages in arxiv. Astrophys Space Sci 367, 115 (2022). The link to the view-only version of my paper is https://rdcu.be/c1daY

References in corpus (58)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
• A Model of Holographic Dark Energy
• BICEP2 I: Detection Of B-mode Polarization at Degree Angular Scales
• Effective Field Theory, Black Holes, and the Cosmological Constant
• Constraints on the redshift dependence of the dark energy potential
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: 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 z$\sim$2
• Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
• Dark Energy
• Two new diagnostics of dark energy
• Black hole thermodynamical entropy
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• A Dark Energy Model Characterized by the Age of the Universe
• A New Model of Agegraphic Dark Energy
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• Tsallis Holographic Dark Energy
• Supernova Constraints on a holographic dark energy model
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
• Dark Interactions and Cosmological Fine-Tuning
• A Note on Tsallis Holographic Dark Energy
• Interacting models of soft coincidence
• Age Problem in the Holographic Dark Energy Model
• Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
• Cosmological dynamics with non-linear interactions
• Observational constraints on interacting Tsallis holographic dark energy models
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• A Critique of Holographic Dark Energy
• Dynamical analysis and statefinder of Barrow holographic dark energy
• Stability analysis of the Tsallis holographic dark energy model
• Tachyon Reconstruction of Ghost Dark Energy
• Cosmic age problem revisited in the holographic dark energy model
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• New Agegraphic Dark Energy in $f(R)$ Gravity
• Effects of Anisotropy on the Sign-Changeable Interacting Tsallis Holographic Dark Energy
• Observational constraint on the interacting dark energy models including the Sandage-Loeb test
• Scrutinizing Various Phenomenological Interactions In The Context Of Holographic Ricci Dark Energy Models
• Note on Tsallis holographic dark energy in Brans-Dicke cosmology
• Tsallis Holographic Dark Energy Reconsidered
• Interacting Tsallis holographic dark energy in higher dimensional Cosmology
• Consistency of nonlinear interacting ghost dark energy with recent observations
• Non-Linearly Interacting Ghost Dark Energy in Brans-Dicke Cosmology
• Interacting Tsallis agegraphic dark energy in DGP Braneworld Cosmology
• Holographic Ricci DE as running vacuum with nonlinear interactions

Cited by in corpus (2)

• Look beyond additivity and extensivity of entropy for black hole and cosmological horizons
• Gravitational wave probes of Barrow cosmology with LISA standard sirens