Class I polytropes for anisotropic matter
arXiv:2103.05039 · doi:10.1140/epjc/s10052-021-09002-1
Abstract
In this work we study class I interior solutions supported by anisotropic polytropes. The generalized Lane--Emden equation compatible with the embedding condition is obtained and solved for a different set of parameters in both the isothermal and non--isothermal regimes. For completeness, the Tolman mass is computed and analysed to some extend. As a complementary study we consider the impact of the Karmarkar condition on the mass and the Tolman mass functions respectively. Comparison with other results in literature are discussed.
References in corpus (32)
- A Large Mass Hierarchy from a Small Extra Dimension
- Decoupling gravitational sources in general relativity: from perfect to anisotropic fluids
- Anisotropic solutions by gravitational decoupling
- Decoupling gravitational sources in general relativity: the extended case
- New definition of complexity for self-gravitating fluid distributions: The spherically symmetric, static case
- General relativistic polytropes for anisotropic matter: The general formalism and applications
- Stability of the isotropic pressure condition
- Study on anisotropic strange stars in gravity: An embedding approach under simplest linear functional of matter-geometry coupling
- Isotropization and change of complexity by gravitational decoupling
- How viscous is a superfluid neutron star core?
- Physically viable solutions of anisotropic spheres in gravity satisfying the Karmarkar condition
- Newtonian polytropes for anisotropic matter: General framework and applications
- Conformally flat polytropes for anisotropic matter
- Anisotropic fluid spheres of embedding class one using Karmarkar condition
- General Relativistic Stars : Polytropic Equations of State
- Karmarkar scalar condition
- Bardeen Stellar Structures with Karmarkar Condition
- A Polytropic Model of Quark Stars
- Cracking of general relativistic anisotropic polytropes
- Bulk Viscosity in Neutron Stars from Hyperons
- A simple method to generate exact physically acceptable anisotropic solutions in general relativity
- Evolution of relativistic polytropes in the post--quasi--static regime
- Anisotropic spheres via embedding approach in gravity with matter coupling
- Relativistic gravitational collapse in non-comoving coordinates: The post-quasistatic approximation
- The Minimal Geometric Deformation Approach: a brief introduction
- A generalized Finch-Skea class one static solution
- Mass-radius relation for magnetized strange quark stars
- The general relativistic double polytrope for anisotropic matter
- The double polytrope for anisotropic matter: Newtonian Case
- No Go Theorem for Kinematic Self-Similarity with A Polytropic Equation of State
- Linear and Riccati equations in generating functions for stellar models in general relativity
- Charged anisotropic compact objects obeying Karmarkar condition
Cited by in corpus (20)
- Uncharged and charged anisotropic like--Durgapal stellar model with vanishing complexity
- Orthogonal splitting of the Riemann curvature tensor and its implications in modeling compact stellar structures
- Charged Anisotropic Models with Complexity-free Condition
- Gravitational decoupling of generalized Horndeski hybrid stars
- Integration of the Lane-Emden equation for relativistic anisotropic polytropes through Gravitational Decoupling: a novel approach
- Gravitational decoupling and superfluid stars
- Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
- Complexity factor for black holes in the framework of the Newman-Penrose formalism
- Complexity factor of spherically anisotropic polytropes from gravitational decoupling
- Axion stars in MGD background
- Gravitational decoupling and aerodynamics: black holes and analog gravity in a jet propulsion lab
- f(R) wormholes embedded in a pseudo--Euclidean space
- Implications of Rastall Theory on Stellar Solutions admitting Vanishing Complexity: A New Perspective
- Double relativistic master polytrope for anisotropic matter
- A Generalized Double Chaplygin Model for Anisotropic Matter: The Newtonian Case
- Relativistic compact stars in Tolman spacetime via an anisotropic approach
- When gravitational decoupling and quantum gravity (re)unite
- Hyperbolic polytrope
- Hair imprints of the gravitational decoupling and hairy black hole spectroscopy
- Gravitational decoupling and regular hairy black holes: Geodesic stability, quasinormal modes, and thermodynamic properties