Models of spherical shells as sources of Majumdar-Papapetrou type spacetimes

DOI10.1007/s10714-017-2197-8zbMath1380.83018arXiv1608.01918OpenAlexW3106368848MaRDI QIDQ682399

Gonzalo García-Reyes

Publication date: 2 February 2018

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1608.01918

zbMATH Keywords

spherical symmetrygeneral relativityenergy conditionsconformastatic spacetimesdisk-haloeshalo of matterMajumdar-Papapetrou-type spacetimes

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)

Cites Work

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• Relativistic dynamics of spherical timelike shells
• Conformastationary disk-haloes in Einstein-Maxwell gravity
• Exact relativistic models of perfect fluid disks in a magnetic field
• The interpretation of some spheroidal metrics
• Gravitational Field of Shells and Disks in General Relativity
• Exact self-gravitating disks and rings: A solitonic approach
• Self-similar relativistic discs with pressure
• On the Distribution of Matter Within Highly Flattened Galaxies.
• Relativistic disks - I. Counter rotating disks
• Exact Solutions of Einstein's Field Equations
• Relativistic disks as sources of the Kerr metric
• THE GENERAL EXACT SOLUTION FOR RELATIVISTIC SPHERICAL SHELLS