Double relativistic master polytrope for anisotropic matter
arXiv:2303.04211 · doi:10.1103/PhysRevD.107.064010
Abstract
We present a detailed analysis of a general relativistic static spherical symmetric distribution in which both the radial and tangential pressures follow a master polytropic equation of state that generalizes the standard treatment and avoids the appearance of singularities in the system. In particular, we find the corresponding Lane-Emden equation and integrate it for a wide range of values of the parameters involved. We explore the parameter space with the aim to find the set of parameters leading to reasonable physical solutions. Also, we considered the effect of spherically symmetric perturbations of the matter variables in order to analyze the possible apparition of cracking within the compact distribution.
References in corpus (20)
- Sound Speeds, Cracking and Stability of Self-Gravitating Anisotropic Compact Objects
- All static spherically symmetric anisotropic solutions of Einstein's equations
- Equation of State of a Dense and Magnetized Fermion System
- Shearing Expansion-free Spherical Anisotropic Fluid Evolution
- Conformally flat polytropes for anisotropic matter
- Analytical study of anisotropic compact star models
- A Polytropic Model of Quark Stars
- Anisotropic Pressures in Very Dense Magnetized Matter
- Bulk viscosity of strange quark matter: Urca versus non-leptonic processes
- A generalized Finch-Skea class one static solution
- The general relativistic double polytrope for anisotropic matter
- Class I polytropes for anisotropic matter
- The double polytrope for anisotropic matter: Newtonian Case
- Bulk viscosity in nuclear and quark matter: A short review
- Timescales for detection of super-Chandrasekhar white dwarfs by gravitational wave astronomy
- Dynamical instability of polytropic spheres in spacetimes with a cosmological constant
- Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
- Acceptability Conditions and Relativistic Barotropic Equations of State
- Polytropic spheres modelling dark matter halos of dwarf galaxies
- Bulk viscosity in 2SC and CFL quark matter