Generating static spherically symmetric anisotropic solutions of Einstein's equations from isotropic Newtonian solutions
arXiv:0905.3546 · doi:10.1103/PhysRevD.80.064039
Abstract
I use the Newtonian equation of hydrostatic equilibrium for an isotropic fluid sphere to generate exact anisotropic solutions of Einstein's equations. The input function is simply the density. An infinite number of regular solutions are constructed, some of which satisfy all the standard energy conditions. Two classes of these solutions generalize the Newtonian polytropes of index 0 and 1.
11 pages, 8 figures, revtex4. Final form to appear in Phys. Rev. D
References in corpus (13)
- Sound Speeds, Cracking and Stability of Self-Gravitating Anisotropic Compact Objects
- All static spherically symmetric anisotropic solutions of Einstein's equations
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- The role of pressure anisotropy on the maximum mass of cold compact stars
- On Einstein clusters as galactic dark matter halos
- Solution generating theorems for the TOV equation
- Sharp bounds on 2m/r for static spherical objects
- Buchdahl-like transformations for perfect fluid spheres
- Modeling usual and unusual anisotropic spheres
- Transforming the Einstein static Universe into physically acceptable static fluid spheres
- Generating Static Fluid Spheres by Conformal Transformations
- Transforming the Einstein static Universe into physically acceptable static fluid spheres II: A two - fold infinity of exact solutions
- Solution generating theorems for perfect fluid spheres