Maximum Mass-Radius Ratios for Charged Compact General Relativistic Objects
arXiv:gr-qc/0107011 · doi:10.1209/epl/i2001-00416-x
Abstract
Upper limits for the mass-radius ratio and total charge are derived for stable charged general relativistic matter distributions. For charged compact objects the mass-radius ratio exceeds the value 4/9 corresponding to neutral stars. General restrictions for the redshift and total energy (including the gravitational contribution) are also obtained.
6 pages, 2 figures, RevTex. To appear in Europhys. Lett
References in corpus (2)
Cited by in corpus (47)
- Anisotropic Stars in General Relativity
- Electrically charged compact stars and formation of charged black holes
- Charged anisotropic matter with linear or nonlinear equation of state
- Sharp bounds on the critical stability radius for relativistic charged spheres
- Strange stars in Krori-Barua space-time
- Nonadiabatic charged spherical gravitational collapse
- Singularity-free dark energy star
- Compact stars in gravity
- Singularity-free solutions for anisotropic charged fluids with Chaplygin equation of state
- Minimum mass-radius ratio for charged gravitational objects
- A relativistic model for Strange Quark Star
- Relativistic stellar model admitting a quadratic equation of state
- Anisotropic strange star with Tolman-Kuchowicz metric under gravity
- Central Density Dependent Anisotropic Compact Stars
- Polytropic spheres with electric charge: compact stars, the Oppenheimer-Volkoff and Buchdahl limits, and quasiblack holes
- A new solution of embedding class I representing anisotropic fluid sphere in general relativity
- Relativistic strange stars in Tolman-Kuchowicz spacetime
- Does the cosmological constant imply the existence of a minimum mass?
- Mass bounds for compact spherically symmetric objects in generalized gravity theories
- Absolute Stability Limit for Relativistic Charged Spheres
- Charged Vaidya-Tikekar model for super compact star
- Quasiblack holes with pressure: relativistic charged spheres as the frozen stars
- Bonnor stars in d spacetime dimensions
- Bounds on M/R for Charged Objects with positive Cosmological constant
- Buchdahl compactness limit and gravitational field energy
- Relativistic Compact Objects in Isotropic Coordinates
- Spherically symmetric models for charged radiating stars and voids: Theoretical approach
- Anisotropic charged dark energy star
- An electromagnetic extension of the Schwarzschild interior solution and the corresponding Buchdahl limit
- The minimum mass of a spherically symmetric object in -dimensions, and its implications for the mass hierarchy problem
- The Stability of a Shearing Viscous Star with Electromagnetic Field
- Relativistic Polytropic Models of Charged Anisotropic Compact Object
- The minimum mass of a charged spherically symmetric object in dimensions, its implications for fundamental particles, and holography
- Analytical model of strange star in the low-mass X-ray binary 4U 1820-30
- Mass - radius ratio bounds for compact objects in Lorentz-violating dRGT Massive Gravity theory
- Radiation Fluid Stars in the Non-minimally Coupled Gravity
- Gyromagnetic ratio of rapidly rotating compact stars in general relativity
- Charged anisotropic compact objects obeying Karmarkar condition
- New bound of the mass-to-radius ratio for electrically charged stars
- Does space-time torsion determine the minimum mass of gravitating particles?
- Anisotropic strange stars with Tolman V potential
- Lack of Debye and Meissner screening in strongly magnetized quark matter at intermediate densities
- Anisotropic Stars in the Non-minimal Gravity
- The QCD mass gap and quark deconfinement scales as mass bounds in strong gravity
- Charged analog of anisotropic dark energy star in Rastall gravity
- Analytical model on mass limit of strange stars
- Gravastars in a Non-minimally Coupled Gravity with Electromagnetism