Two Fluid Shear-Free Composites
arXiv:1307.1080 · doi:10.1063/1.4815976
Abstract
Shear-free composite fluids are constructed from two Letelier rotated unaligned perfect fluids. The component fluid parameters necessary to construct a shear-free composite are investigated. A metric in the Stephani-Barnes solution family and a simple stationary metric are discussed.
misprints corrected, J. Math. Physics (to appear)
References in corpus (13)
- Shearing Expansion-free Spherical Anisotropic Fluid Evolution
- Thermal Dynamics in General Relativity
- Two-fluid models of superfluid neutron star cores
- Oscillations of General Relativistic Multi-fluid/Multi-layer Compact Stars
- Magnetic Field Evolution in Neutron Stars: One-Dimensional Multi-Fluid Model
- Two-fluid dark matter models
- Dark energy interacting with two fluids
- Shearfree perfect fluids with solenoidal magnetic curvature and a gamma-law equation of state
- Cosmological solutions of the Einstein equation with heat flow
- Non-adiabatic perturbations in multi-component perfect fluids
- Two-Component Cosmological Fluids with Gravitational Instabilities
- Mathisson's helical motions demystified
- Non-spherical collapse of a two fluid star
Cited by in corpus (7)
- Stellar models with like--Tolman IV complexity factor
- Cracking of general relativistic anisotropic polytropes
- Gravitational cracking and complexity in the framework of gravitational decoupling
- All static spherically symmetric anisotropic solutions for general relativistic polytropes
- Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
- Double relativistic master polytrope for anisotropic matter
- Collapse in gravity and the method of matching