Results 31 to 40 of about 738,435 (332)

Rip Cosmology via Inhomogeneous Fluid

open access: yesGalaxies, 2013
The conditions for the appearance of the Little Rip, Pseudo Rip and Quasi Rip universes in the terms of the parameters in the equation of state of some dark fluid are investigated. Several examples of the Rip cosmologies are investigated.
Alexander V. Timoshkin   +2 more
doaj   +1 more source

Dark sector unifications: Dark matter-phantom energy, dark matter - constant w dark energy, dark matter-dark energy-dark matter

open access: yesPhysics Letters B, 2019
The paper brings a novel approach to unification of dark matter and dark energy in terms of a cosmic fluid. A model is introduced in which the cosmic fluid speed of sound squared is defined as a function of its equation of state (EoS) parameter.
Dalibor Perković, Hrvoje Štefančić
doaj   +1 more source

Vacuum dark fluid

open access: yesPhysics Letters B, 2007
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Dymnikova, Irina, Galaktionov, Evgeny
openaire   +2 more sources

Dark radiation from a unified dark fluid model [PDF]

open access: yesProgress of Theoretical and Experimental Physics, 2014
We present a unified dark fluid model to describe the possible evolutionary behavior of $ N_\mathrm{eff}$ in dark radiation. This model can be viewed as an interacting model for the dark sectors, in which dark matter interacts with dark radiation. We show that the evolution of $ N_\mathrm{eff}$ can be nicely explained without some drawbacks, such as ...
Geng, Chao-Qiang   +2 more
openaire   +2 more sources

Kerr–Newman-AdS black hole surrounded by perfect fluid matter in Rastall gravity

open access: yesEuropean Physical Journal C: Particles and Fields, 2018
The Rastall gravity is the modified Einstein general relativity, in which the energy-momentum conservation law is generalized to $$T^{\mu \nu }_{~~;\mu }=\lambda R^{,\nu }$$ T;μμν=λR,ν .
Zhaoyi Xu   +3 more
doaj   +1 more source

Instability and phase transitions of a rotating black hole in the presence of perfect fluid dark matter

open access: yesEuropean Physical Journal C: Particles and Fields, 2020
In this paper, we study the thermodynamic features of a rotating black hole surrounded by perfect fluid dark matter. We analyze the critical behavior of the black hole by considering the known relationship between pressure and cosmological constant.
Seyed Hossein Hendi   +3 more
doaj   +1 more source

A viable dark fluid model [PDF]

open access: yesAstrophysics and Space Science, 2017
We Consider a cosmological model based on a generalization of the equation of state proposed by Nojiri and Odintsov [46] and Štefanči'c [47], [48]. We argue that this model works as a dark fluid model which can interpolate between dust equation of state and the dark energy equation of state.
openaire   +2 more sources

Dark energy coupled with dark matter in viscous fluid cosmology [PDF]

open access: yesAstrophysics and Space Science, 2014
6 pages, no figures; to appear in Astrophys.
Brevik, I.   +2 more
openaire   +2 more sources

Dark energy and dark matter from an additional adiabatic fluid [PDF]

open access: yesPhysical Review D, 2016
The Dark Sector is described by an additional barotropic fluid which evolves adiabatically during the universe's history and whose adiabatic exponent $ $ is derived from the standard definitions of specific heats. Although in general $ $ is a function of the redshift, the Hubble parameter and its derivatives, we find that our assumptions lead ...
Dunsby, Peter K. S.   +2 more
openaire   +2 more sources

Darkness without dark matter and energy – generalized unimodular gravity

open access: yesPhysics Letters B, 2017
We suggest a Lorentz non-invariant generalization of the unimodular gravity theory, which is classically equivalent to general relativity with a locally inert (devoid of local degrees of freedom) perfect fluid having an equation of state with a constant ...
A.O. Barvinsky, A.Yu. Kamenshchik
doaj   +1 more source

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