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Journal ArticleDOI

Various aspects of interacting modified holographic Ricci dark energy

Surajit Chattopadhyay, +1 more
- 28 May 2013 - 
- Vol. 87, Iss: 10, pp 1053-1057
TLDR
In this article, the authors reported various aspects of modified holographic Ricci dark energy interacting with pressureless dark matter in a flat Friedman-Robertson-Walker universe, and the cosmological parameters, namely, Hubble parameter, equation of state parameter and deceleration parameter have been studied under this interaction.
Abstract
The present paper reports various aspects of modified holographic Ricci dark energy interacting with pressureless dark matter in a flat Friedman-Robertson-Walker universe. The cosmological parameters, namely, Hubble parameter, equation of state parameter and deceleration parameter have been studied under this interaction. Statfinder diagnostics has also been studied, where attainment of $$\Uplambda$$ CDM phase of the universe under this interaction has been observed. A study on fractional densities has prominently shown the transition from matter dominated to dark energy dominated universe.

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Citations
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Journal ArticleDOI

A Rindler-KAM Spacetime Geometry and Scaling the Planck Scale Solves Quantum Relativity and Explains Dark Energy

TL;DR: In this paper, an ultra high======energy combined KAM-Rindler fractal spacetime quantum manifold, which increasingly resembles Einstein's smooth relativity spacetime, with decreasing energy, was introduced.
Journal ArticleDOI

Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi Type I universe

TL;DR: In this paper, the generalized second law of thermodynamics in the Bianchi Type I universe with the generalized holographic Ricci dark energy model is studied and the behavior of dark energy's equation of state parameter indicates that it is matterlike in the early time of the universe but phantom-like in future.
Journal ArticleDOI

QCD ghost reconstruction of f(T) gravity in flat FRW universe

TL;DR: In this paper, a reconstruction scheme for f(T) gravity based on QCD ghost dark energy has been reported, and two realistic models have been obtained and the effective equations of state have been studied.
Journal ArticleDOI

On the Dynamics of Dark Energy with Higher Time Derivatives of Hubble Parameter in El-Nabulsi Fractional Action Cosmology

TL;DR: In this paper, a new dark energy density model which contains one term proportional to the Hubble parameter H squared, one to the first and one to second time derivative of the Hubble parameters H based on El-Nabulsi fractional action cosmology (FAC) was discussed.
Journal ArticleDOI

Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory

TL;DR: In this paper, Kumar et al. reported a study on the viscous extended holographic Ricci dark energy (EHRDE) model under the assumption of existence of bulk viscosity in the linear barotropic fluid and the EHRDE in the framework of standard Eckart theory of relativistic irreversible thermodynamics and observed that the non-equilibrium bulk viscous pressure is significantly smaller than the local equilibrium pressure.
References
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Journal ArticleDOI

Dynamics of dark energy

TL;DR: In this article, the authors review the observational evidence for the current accelerated expansion of the universe and present a number of dark energy models in addition to the conventional cosmological constant, paying particular attention to scalar field models such as quintessence, K-essence and tachyon.
Journal ArticleDOI

Cosmological constant—the weight of the vacuum

TL;DR: A review of cosmological constants can be found in this paper, where the authors discuss several aspects of the Cosmological Constant problem from both cosmology and theoretical perspectives.
Journal ArticleDOI

A model of holographic dark energy

TL;DR: In this article, a model for holographic dark energy is proposed, following the idea that the short distance cutoff is related to the infrared cut-off, and the model predicts the equation of state of the dark energy at the present time to be characterized by w = -0.90.
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