We have reexamined the holographic dark energy model by considering the spatial curvature. We have refined the model parameter and observed that the holographic dark energy model does not behave as phantom. Applying the holographic dark energy model and comparing to the supernova observation alone, we found that the closed universe is favored. Combining with the WMAP data, we obtained the reasonable value of the spatial curvature of our universe
Abstract The model of holographic dark energy in which dark energy interacts with dark matter is inv...
Doctor of PhilosophyDepartment of PhysicsBharat RatraObservations conducted over the last few decade...
AbstractWe investigate canonical, phantom and quintom models, with the various fields being non-mini...
In this paper we place observational constraints on the interaction and spatial curvature in the hol...
In this paper, we report the results of constraining the holographic dark energy model with spatial ...
We study the model for holographic dark energy in a spatially closed universe, generalizing the prop...
We propose an alternative model for the holographic dark energy in a non-flat universe. This new mod...
M R Setare et al study the holographic dark energy model in a non-flat universe from the statefinder...
We propose an alternative model for the holographic dark energy in a non-flat universe. This new mod...
In this paper, we study the holographic dark energy model in non-flat universe from the statefinder ...
Motivated by recent results on non-vanishing spatial curvature \cite{curve} we employ the holographi...
In this work we explore the scope of two holographic dark energy models within the interacting scena...
We study the perturbation of holographic dark energy and find it to be stable. We study the fate of ...
We investigate the accelerated expansion of the late-time universe in the Friedmann-Robertson-Walker...
Employing the modified entropy–area relation suggested by Tsallis and Cirto [1], and the holographic...
Abstract The model of holographic dark energy in which dark energy interacts with dark matter is inv...
Doctor of PhilosophyDepartment of PhysicsBharat RatraObservations conducted over the last few decade...
AbstractWe investigate canonical, phantom and quintom models, with the various fields being non-mini...
In this paper we place observational constraints on the interaction and spatial curvature in the hol...
In this paper, we report the results of constraining the holographic dark energy model with spatial ...
We study the model for holographic dark energy in a spatially closed universe, generalizing the prop...
We propose an alternative model for the holographic dark energy in a non-flat universe. This new mod...
M R Setare et al study the holographic dark energy model in a non-flat universe from the statefinder...
We propose an alternative model for the holographic dark energy in a non-flat universe. This new mod...
In this paper, we study the holographic dark energy model in non-flat universe from the statefinder ...
Motivated by recent results on non-vanishing spatial curvature \cite{curve} we employ the holographi...
In this work we explore the scope of two holographic dark energy models within the interacting scena...
We study the perturbation of holographic dark energy and find it to be stable. We study the fate of ...
We investigate the accelerated expansion of the late-time universe in the Friedmann-Robertson-Walker...
Employing the modified entropy–area relation suggested by Tsallis and Cirto [1], and the holographic...
Abstract The model of holographic dark energy in which dark energy interacts with dark matter is inv...
Doctor of PhilosophyDepartment of PhysicsBharat RatraObservations conducted over the last few decade...
AbstractWe investigate canonical, phantom and quintom models, with the various fields being non-mini...