Conformally flat polytropes for anisotropic matter
arXiv:1410.6636 · doi:10.1007/s10714-014-1827-7
Abstract
We analyze in detail conformally flat spherically symmetric fluid distributions, satisfying a polytropic equation of state. Among the two possible families of relativistic polytropes, only one contains models which satisfy all the required physical conditions. The ensuing configurations are necessarily anisotropic and show interesting physical properties. Prospective applications of the presented models to the study of super-Chandrasekhar white dwarfs, are discussed.
9 pages Revtex-4, 6 figures. To appear in Gen. Rel. Grav. Some typos corrected
References in corpus (32)
- The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star
- Maximum bounds on the surface redshift of anisotropic stars
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- Nearby Supernova Factory Observations of SN 2007if: First Total Mass Measurement of a Super-Chandrasekhar-Mass Progenitor
- Equation of State of a Dense and Magnetized Fermion System
- The Luminous and Carbon-Rich Supernova 2006gz: A Double Degenerate Merger?
- General relativistic polytropes for anisotropic matter: The general formalism and applications
- Fourteen Months of Observations of the Possible Super-Chandrasekhar Mass Type Ia Supernova 2009dc
- High luminosity, slow ejecta and persistent carbon lines: SN 2009dc challenges thermonuclear explosion scenarios
- Sharp bounds on of general spherically symmetric static objects
- On the role of density inhomogeneity and local anisotropy in the fate of spherical collapse
- Conformally flat anisotropic spheres in general relativity
- Early phase observations of extremely luminous Type Ia Supernova 2009dc
- New mass limit for white dwarfs: super-Chandrasekhar type Ia supernova as a new standard candle
- Quantum Magnetic Collapse
- Newtonian polytropes for anisotropic matter: General framework and applications
- Magnetic collapse of a neutron gas: Can magnetars indeed be formed
- The role of pressure anisotropy on the maximum mass of cold compact stars
- Strongly magnetized cold electron degenerate gas: Mass-radius relation of the magnetized white dwarf
- Spherically symmetric relativistic stellar structures
- Anisotropic Pressures in Very Dense Magnetized Matter
- Space-time inhomogeneity, anisotropy and gravitational collapse
- Sharp bounds on 2m/r for static spherical objects
- Local conditions separating expansion from collapse in spherically symmetric models with anisotropic pressures
- Neutron stars in a perturbative gravity model with strong magnetic fields
- Evolution of the density contrast in inhomogeneous dust models
- A possible evolutionary scenario of highly magnetized super-Chandrasekhar white dwarfs: progenitors of peculiar type Ia supernovae
- Mass of highly magnetized white dwarfs exceeding the Chandrasekhar limit: An analytical view
- Violation of Chandrasekhar Mass Limit: The Exciting Potential of Strongly Magnetized White Dwarfs
- One possible solution of peculiar type Ia supernovae explosions caused by a charged white dwarf
- Revisiting some physics issues related to the new mass limit for magnetized white dwarfs
- New mass limit of white dwarfs
Cited by in corpus (37)
- Role of pressure anisotropy on relativistic compact stars
- Analytical study of anisotropic compact star models
- A conformally flat realistic anisotropic model for a compact star
- Cracking of general relativistic anisotropic polytropes
- Uncharged and charged anisotropic like--Durgapal stellar model with vanishing complexity
- Buchdahl-Bondi limit in modified gravity: Packing extra effective mass in relativistic compact stars
- Role of gravitational decoupling on isotropization and complexity of self-gravitating system under complete geometric deformation approach
- Charged Anisotropic Models with Complexity-free Condition
- The general relativistic double polytrope for anisotropic matter
- Class I polytropes for anisotropic matter
- The double polytrope for anisotropic matter: Newtonian Case
- Study of polytropes with Generalized polytropic Equation of State
- GRMHD formulation of highly super-Chandrasekhar magnetized white dwarfs: stable configurations of non-spherical white dwarfs
- On the maximum mass of magnetised white dwarfs
- Role of Non-conserved Gravity Theory and Electric Charge in Constructing Complexity-free Stellar Models: A Novel Approach under Non-minimal Coupling
- Integration of the Lane-Emden equation for relativistic anisotropic polytropes through Gravitational Decoupling: a novel approach
- All static spherically symmetric anisotropic solutions for general relativistic polytropes
- Linear and Riccati equations in generating functions for stellar models in general relativity
- Cracking of Charged Polytropes with Generalized Polytropic Equation of State
- Electromagnetic Effects on Cracking of Anisotropic Polytropes
- Charged Cylindrical Polytropes with Generalized Polytropic Equation of State
- Analytical model of dark energy stars
- Anisotropic solution for polytropic stars in 4D Einstein-Gauss-Bonnet gravity
- Complexity factor for black holes in the framework of the Newman-Penrose formalism
- Gravitational Cracking of General Relativistic Polytropes: a generalized scheme
- Complexity factor of spherically anisotropic polytropes from gravitational decoupling
- On Cracking of Charged Anisotropic Polytropes
- Implications of Rastall Theory on Stellar Solutions admitting Vanishing Complexity: A New Perspective
- Double relativistic master polytrope for anisotropic matter
- Relativistic polytropic equations of state in Hořava gravity and Einstein-æther theory
- Complexity Factor for Static Cylindrical System in Energy-momentum Squared Gravity
- Study of Complexity Factor and Stability of Dynamical Systems in Gravity
- Development of complexity induced frameworks for charged cylindrical polytropes
- Role of Model on Anisotropic Polytropes
- Hyperbolic polytrope
- Series solutions to the TOV equations
- Self-Gravitating Relativistic Models of Fermions with Anisotropy and Cutoff Energy in their Distribution Function