All static spherically symmetric anisotropic solutions for general relativistic polytropes
arXiv:1905.05378 · doi:10.1142/S0218271820500820
Abstract
An algorithm presented by K. Lake to obtain all static spherically symmetric perfect fluid solutions was recently extended by L. Herrera to the interesting case of locally anisotropic fluids (principal stresses unequal). In this work we develop an algorithm to construct all static spherically symmetric anisotropic solutions for general relativistic polytropes. Again the formalism requires the knowledge of only one function (instead of two) to generate all possible solutions. To illustrate the method some known cases are recovered.
Figures added, new section added
References in corpus (16)
- All static spherically symmetric anisotropic solutions of Einstein's equations
- Stability of the isotropic pressure condition
- Study on anisotropic strange stars in gravity: An embedding approach under simplest linear functional of matter-geometry coupling
- Shearing Expansion-free Spherical Anisotropic Fluid Evolution
- Conformally flat polytropes for anisotropic matter
- A general interior anisotropic solution for a BTZ vacuum in the context of the Minimal Geometric Deformation decoupling approach
- Karmarkar scalar condition
- A Polytropic Model of Quark Stars
- Exact power series solutions of the structure equations of the general relativistic isotropic fluid stars with linear barotropic and polytropic equations of state
- Bulk viscosity of strange quark matter: Urca versus non-leptonic processes
- Generating static spherically symmetric anisotropic solutions of Einstein's equations from isotropic Newtonian solutions
- A generalized Finch-Skea class one static solution
- The general relativistic double polytrope for anisotropic matter
- The double polytrope for anisotropic matter: Newtonian Case
- Bulk viscosity in nuclear and quark matter: A short review
- Bulk viscosity in 2SC and CFL quark matter
Cited by in corpus (10)
- Charged Anisotropic Models with Complexity-free Condition
- Role of Non-conserved Gravity Theory and Electric Charge in Constructing Complexity-free Stellar Models: A Novel Approach under Non-minimal Coupling
- Modelling a Compact Star with Quark Matter
- Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
- Acceptability Conditions and Relativistic Barotropic Equations of State
- Acceptability Conditions and Relativistic Anisotropic Generalized Polytropes
- Implications of Rastall Theory on Stellar Solutions admitting Vanishing Complexity: A New Perspective
- Double relativistic master polytrope for anisotropic matter
- Hyperbolic Casimir-like wormhole
- Hyperbolic polytrope