Generating static perfect-fluid solutions of Einstein’s equations [PDF]
We present a method for generating exact interior solutions of Einstein’s equations in the case of static and axially symmetric perfect-fluid spacetimes. The method is based upon a transformation that involves the metric functions as well as the density and pressure of the seed solution.
Hernando Quevedo, Saken Toktarbay
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Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations [PDF]
We ask the following question: Of the exact solutions to Einstein's equations extant in the literature, how many could represent the field associated with an isolated static spherically symmetric perfect fluid source? The candidate solutions were subjected to the following elementary tests: i) isotropy of the pressure, ii) regularity at the origin, iii)
Delgaty, M. S. R., Lake, Kayll
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Static perfect fluids with Pant-Sah equations of state [PDF]
32 p., Latex, minor changes and ...
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All static spherically symmetric perfect-fluid solutions of Einstein’s equations [PDF]
Final form to appear in Phys Rev D.
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Static spherically symmetric Einstein-aether models I: perfect fluids with a linear equation of state and scalar fields with an exponential self-interacting potential [PDF]
46 pages, 4 compound figures.
Alan Coley, Genly Leon
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On Minimal Hypersurfaces of a Unit Sphere
Minimal compact hypersurface in the unit sphere Sn+1 having squared length of shape operator A22), provided the scalar curvature τ is a constant on integral curves of w.
Amira Ishan +3 more
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General exact solutions of Einstein equations for static perfect fluids with spherical symmetry
The gravitational field equations for a spherical symmetric perfect fluid are completely solved. The general analytical solution obtained depends on an arbitrary function of the radial coordinate. As illustrations of the proposed procedure the exterior and interior Schwarzschild solutions are regained.
Berger, Sonia +2 more
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On the stability of Einstein static universe at background level in massive bigravity
We study the static cosmological solutions and their stability at background level in the framework of massive bigravity theory with Friedmann–Robertson–Walker (FRW) metrics. By the modification proposed in the cosmological equations subject to a perfect
M. Mousavi, F. Darabi
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Cylindrically Symmetric, Static, Perfect-Fluid Solutions of Einstein's Field Equations
Perfect-fluid, static, cylindrically symmetric solutions of Einstein's field equations are obtained for the equations of state $ρ+3p=0$ and $ρ=p$. In the former case, the density and the pressure turn out to be constant while in the later case, they depend on the radial parameter $r$.
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Fluid black holes with electric field
We investigate the gravitational field of static perfect-fluid in the presence of electric field. We adopt the equation of state $$p(r)=-\rho (r)/3$$ p(r)=-ρ(r)/3 for the fluid in order to consider the closed ($$S_3$$ S3 ) or the open ($$H_3$$ H3 ...
Inyong Cho
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