Acceptability Conditions and Relativistic Anisotropic Generalized Polytropes
arXiv:2104.08923 · doi:10.1140/epjc/s10052-022-10119-0
Abstract
This paper explored the physical acceptability conditions for anisotropic matter configurations in General Relativity. The study considered a generalized polytropic equation of state for a heuristic anisotropy. We integrated the corresponding Lane-Emden equation for several hundred models and found the parameter-space portion ensuring the configurations' acceptability. Polytrope based on the total energy density are more stable than those with baryonic density, and small positive local anisotropies produce acceptable models. We also found that polytropic configurations where tangential pressures are greater than radial ones are also more acceptable. Finally, convective disturbances do not generate cracking instabilities. Several models emerging from our simulations could represent candidate of astrophysical compact objects.
31 pages, 11 figures
References in corpus (24)
- Multi-messenger Observations of a Binary Neutron Star Merger
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- Tidal Love numbers of neutron stars
- Constraining neutron star tidal Love numbers with gravitational wave detectors
- Sound Speeds, Cracking and Stability of Self-Gravitating Anisotropic Compact Objects
- Relativistic theory of tidal Love numbers
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- All static spherically symmetric anisotropic solutions of Einstein's equations
- Stability of the isotropic pressure condition
- Non-radial oscillations of anisotropic neutron stars in the Cowling approximation
- Radial pulsations and stability of anisotropic stars with quasi-local equation of state
- Analytical study of anisotropic compact star models
- Multi-telescope timing of PSR J1518+4904
- Dissipative collapse of axially symmetric, general relativistic, sources: A general framework and some applications
- The tidal deformability of an anisotropic compact star: Implications of GW170817
- The general relativistic double polytrope for anisotropic matter
- Anisotropic compact stars: Constraining model parameters to account for physical features of tidal Love numbers
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
- Where is Love? Tidal deformability in the black hole compactness limit
- Tidal deformability and radial oscillations of anisotropic polytropic spheres
- Acceptability Conditions and Relativistic Barotropic Equations of State
- Neutron and quark stars: constraining the parameters for simple EoS using the GW170817
- Relativistic Anisotropic Polytropic Spheres: Physical Acceptability
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