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Conformal Einstein Perfect Fluid Spacetimes [PDF]
A review is given of results obtained in connection with perfect fluid spacetimes which are conformally related to Einstein spaces.
Norbert Van den Bergh +1 more
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Kerr–Newman-AdS black hole surrounded by perfect fluid matter in Rastall gravity
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
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Gradient Ricci Bourguignon solitons on perfect fluid space-times [PDF]
The main purpose of the present paper is about characterizing the properties of the perfect fluid space-time that admits the gradient Ricci-Bourguignon soliton. This gives some results about the stability of the energy-momentum tensor and also under some
Sakineh Hajiaghasi, Shahroud Azami
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7 pages, 5 figures, To appear in Phys. Lett. B (2010)
Rahaman, F. +4 more
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Conformally Flat Pseudoprojective Symmetric Spacetimes in fR,G Gravity
Sufficient conditions on a pseudoprojective symmetric spacetime PPSn whose Ricci tensor is of Codazzi type to be either a perfect fluid or Einstein spacetime are given.
Uday Chand De +3 more
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Graphene: A Nearly Perfect Fluid [PDF]
Hydrodynamics and collision-dominated transport are crucial to understand the slow dynamics of many correlated quantum liquids. The ratio eta/s of the shear viscosity eta to the entropy density s is uniquely suited to determine how strongly the excitations in a quantum fluid interact. We determine eta/s in clean undoped graphene using a quantum kinetic
Markus, Müller +2 more
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Solution Generating with Perfect Fluids [PDF]
We apply a technique, due to Stephani, for generating solutions of the Einstein-perfect fluid equations. This technique is similar to the vacuum solution generating techniques of Ehlers, Harrison, Geroch and others. We start with a ``seed'' solution of the Einstein-perfect fluid equations with a Killing vector.
Garfinkle, David +2 more
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Perfect fluid spacetimes with two symmetries [PDF]
A method of solving perfect fluid Einstein equations with two commuting spacelike Killing vectors is presented. Given a spacelike 2-dimensional surface in the 3-dimensional nonphysical Minkowski space the field equations reduce to a single nonlinear differential equation. An example is discussed.
Szereszewski, A., Tafel, J.
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Cosmological constant as Hyper Geometric function in fivedimensional space-time
In this paper, we have studied the Einstein Field equation in Kaluza-Klein space-time in five dimension with the metric dS^2 = dt^2 − A^2(dx^2 + dy^2 + dz^2)− B^2dψ^2 under the assumption that B = αt, where α = Constant and scale factor satisfying the ...
Satish T. Rathod, Kalpana Pawar
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Axistationary perfect fluids - a tetrad approach [PDF]
12 ...
Fodor, Gyula +2 more
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