Sharp bounds on the critical stability radius for relativistic charged spheres

From MaRDI portal
Publication:842466

DOI10.1007/s00220-008-0690-3zbMath1175.83015arXiv0804.1882OpenAlexW3100359061MaRDI QIDQ842466

Håakan Andréasson

Publication date: 25 September 2009

Published in: Communications in Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0804.1882




Related Items (50)

Massive compact Bardeen stars with conformal motionAnisotropic quintessence strange stars in \(f(T)\) gravity with modified Chaplygin gasRastall-Maxwell approach for anisotropic charged strange starsBuchdahl type inequalities in d dimensionsStructural properties of charged compact stars with color-flavor-locked quarks matterDetermination of the charge for strange starsBuchdahl compactness limit and gravitational field energyAn exact family of Einstein-Maxwell Wyman-Adler solution in general relativityAnisotropic spherical solutions through extended gravitational decoupling approachMass-radius ratio bound for horizonless charged compact object in higher dimensionsRelativistic Krori‐Barua Compact Stars in f(R,T)$f(R,T)$ GravityRelativistic charged stellar modeling with a perfect fluid sphereRelativistic model for anisotropic strange starsStrange stars in Krori-Barua spacetime under \(f(R,T)\) gravityAnisotropic stellar compact spheres in f(R) gravity via Karmarkar approachAnisotropic compact star models in f(T) gravity with Tolman–Kuchowicz spacetimeCompact stars described by a charged modelBardeen compact stars in modified f(R) gravity with conformal motionCompact Bardeen Stars in f(R,T)$f(\mathcal {R}, T)$ Theory with Conformal MotionA charged perfect fluid solutionElectromagnetic effects on the stability of anisotropic cylinderAn anisotropic model for starsA new class of relativistic model of compact stars of embedding class IHigher dimensional extension of charged and neutral fluid spheres with pressureCharged analogues of Schwarzschild interior solution in terms of pressureSome exact relativistic models of electrically charged self-bound starsA family of well behaved charge analogues of Durgapal's perfect fluid exact solution in general relativityCharged perfect fluids in the presence of a cosmological constantA new well behaved class of charge analogue of Adler's relativistic exact solutionHybrid star model with quark matter and baryonic matter in minimally coupled \(f ( R )\) gravityAnisotropic compact stellar model of embedding class-I satisfying Karmarkar's condition in Vaidya and Tikekar spheroidal geometryA numerical stability analysis for the Einstein–Vlasov systemBekenstein's generalized second law of thermodynamics: the role of the hoop conjectureA lower bound on the Bekenstein-Hawking temperature of black holesUpper bound on the center-of-mass energy of the collisional Penrose processThe Einstein-Vlasov system/kinetic theoryAnisotropic charged strange stars in Krori-Barua spacetime under \(f(R,T)\) gravityEmbedded class-i solution of compact stars in \(f(R)\) gravity with Karmarkar conditionAn analytical anisotropic compact stellar model of embedding class IA study on charged compact starsMathematical Model of Relativistic Anisotropic Compact Stellar Model Admitting Linear Equation of StateStudy on anisotropic strange stars in Rastall gravityModeling of compact stars: an anisotropic approachExistence of Static Solutions of the Einstein--Vlasov--Maxwell System and the Thin Shell LimitElectrically charged strange quark stars with anisotropic matter: exact analytical solutionAn isotropic analytical model for charged starsRelativistic strange stars in Tolman-Kuchowicz spacetimeUltra-compact spherically symmetric dark matter charged star objectsStatic Solutions to the Einstein--Vlasov System with a Nonvanishing Cosmological ConstantECO-spotting: looking for extremely compact objects with bosonic fields



Cites Work


This page was built for publication: Sharp bounds on the critical stability radius for relativistic charged spheres