Results 61 to 70 of about 3,373,254 (352)

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

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

Non-adiabatic dark fluid cosmology [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2009
We model the dark sector of the cosmic substratum by a viscous fluid with an equation of state $p=- $, where $ $ is the fluid-expansion scalar and $ $ is the coefficient of bulk viscosity for which we assume a dependence $ \propto ^ $ on the energy density $ $.
Hipolito-Ricaldi, W.S.   +2 more
openaire   +5 more sources

Observational constraints and predictions of the interacting dark sector with field-fluid mapping [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2021
We consider an interacting field theory model that describes the interaction between dark energy-dark matter interaction. Only for a specific interaction term, this interacting field theory description has an equivalent interacting fluid description. For
Joseph P. Johnson   +2 more
semanticscholar   +1 more source

Supermassive black holes surrounded by dark matter modeled as anisotropic fluid: epicyclic oscillations and their fitting to observed QPOs [PDF]

open access: yes, 2021
Recently introduced exact solution of the Einstein gravity coupled minimally to an anisotropic fluid representing dark matter can well represent supermassive black holes in galactic nuclei with realistic distribution of dark matter around the black hole,
Zdenvek Stuchl'ik, J. Vrba
semanticscholar   +1 more source

Dark energy with logarithmic cosmological fluid [PDF]

open access: yesJournal of the Korean Physical Society, 2014
14 pages, 1 figure, to be published in The Journal of the Korean Physical ...
Phillial Oh, Seyen Kouwn, Seyen Kouwn
openaire   +3 more sources

Two-fluid dark matter models [PDF]

open access: yesPhysical Review D, 2011
6 pages, two figures, accepted for publication in ...
Lobo, FSN, Harko, T
openaire   +5 more sources

Testing the weak cosmic censorship conjecture for a Reissner–Nordström–de Sitter black hole surrounded by perfect fluid dark matter

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
In this paper, we test the weak cosmic censorship conjecture (WCCC) for the Reissner–Nordström–de Sitter (RN-dS) black hole surrounded by perfect fluid dark matter.
Sanjar Shaymatov   +2 more
doaj   +1 more source

Galactic halos of fluid dark matter [PDF]

open access: yesPhysical Review D, 2003
Dwarf spiral galaxies - and in particular the prototypical DDO 154 - are known to be completely dominated by an unseen component. The putative neutralinos - so far the favored explanation for the astronomical dark matter - fail to reproduce the well measured rotation curves of those systems because these species tend to form a central cusp whose ...
Arbey, Alexandre   +2 more
openaire   +3 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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