Sharp bounds on the radius of relativistic charged spheres: Guilfoyle's stars saturate the Buchdahl–Andréasson bound

DOI10.1088/0264-9381/32/13/135009zbMath1323.83007arXiv1505.03863OpenAlexW3104699291MaRDI QIDQ3447542

Vilson T. Zanchin, José P. S. Lemos

Publication date: 27 October 2015

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1505.03863

zbMATH Keywords

relativistic starsBuchdahl limitcharged starsSchwarzschild interior limit

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

Related Items (3)

Buchdahl compactness limit and gravitational field energy ⋮ Compact stars described by a charged model ⋮ Weakly charged compact stars in f(R) gravity

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