Bertotti–Robinson and Melvin spacetimes

DOI10.1088/0264-9381/28/21/215012zbMath1230.83028arXiv1109.1535OpenAlexW2055239566MaRDI QIDQ3102273

E. N. Glass, David Garfinkle

Publication date: 2 December 2011

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

Full work available at URL: https://arxiv.org/abs/1109.1535

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Global differential geometry of Lorentz manifolds, manifolds with indefinite metrics (53C50) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

Related Items (2)

Spin-induced scalarization and magnetic fields ⋮ Hairy extension of the Bertotti–Robinson spacetime in the Einstein–Maxwell-scalar theory is a black hole in closed spatial geometries

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