EVOLVING SPHERES OF SHEAR-FREE ANISOTROPIC FLUID
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Publication:3590722
DOI10.1142/S0217751X10050202zbMath1194.83055arXiv1103.4225WikidataQ124925734 ScholiaQ124925734MaRDI QIDQ3590722
Publication date: 13 September 2010
Published in: International Journal of Modern Physics A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1103.4225
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)
Related Items (4)
Compact stellar model in higher torsion gravitational theory ⋮ A new class of analytical solutions describing anisotropic neutron stars in general relativity ⋮ Evolution of expansion-free spherically symmetric self-gravitating non-dissipative fluids and some analytical solutions ⋮ Collapsing shear-free perfect fluid spheres with heat flow
Cites Work
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- Shear-free spherically symmetric solutions with conformal symmetry
- The importance of anisotropy for relativistic fluids with spherical symmetry
- Perfect fluid spheres in general relativity
- On the gravitational motion of a fluid obeying an equation of state
- Singularities in gravitational collapse with radial pressure
- On shear-free motion of charged perfect fluid obeying an equation of state in general relativity
- Expanding spherically symmetric models without shear
- Comment: On charged analogue of shear-free fluids
- Über Lösungen der Einsteinschen Feldgleichungen, die sich in einen fünfdimensionalen flachen Raum einbetten lassen
- Charged sphere of shear-free fluids with \(\frac{\partial\rho}{\partial r} \leq 0\)
- Solvable models of relativistic charged spherically symmetric fluids
- Conformally flat anisotropic spheres in general relativity
- Cosmological solution of Einstein’s equations with uniform density and nonuniform pressure
- A new interior solution of Einstein's field equations for a spherically symmetric perfect fluid in shear-free motion
- Perturbative quantum corrections and flux compactifications
- On spherically symmetric shear-free perfect fluid configurations (neutral and charged). I
- Exact solutions for shear-free motion of spherically symmetric perfect fluid distributions in general relativity
- Spherical gravitational collapse with tangential pressure
- Jeffery-Williams Lecture, 1976 Non-Static Radially Symmetric Distributions of Matter
- On the cosmic censorship conjecture for spherically symmetric, shear-free perfect fluid spacetimes
- The Mass-Particle in an Expanding Universe
- Shear-free relativistic fluids and the absence of movable branch points
- Spherically symmetric perfect fluids in shear-free motion - the symmetry approach
- RADIATING COLLAPSE WITH VANISHING WEYL STRESSES
- The contraction of gravitating spheres
- Time-Dependent Internal Solutions for Spherically Symmetrical Bodies in General Relativity: II. Adiabatic Radial Motions of Uniformly Dense Spheres
- Spherical Symmetry and Mass-Energy in General Relativity. I. General Theory
- Some properties of a uniform fluid sphere in general relativity
- SHEAR-FREE RADIATING COLLAPSE AND CONFORMAL FLATNESS
- On shear-free motion of charged perfect fluid obeying an equation of state in general relativity
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