Planar and axisymmetric walls in general relativity, a comparison

DOI10.1063/1.530433zbMath0809.53086OpenAlexW2050223296MaRDI QIDQ4317970

O. S. Ventura, José P. S. Lemos

Publication date: 30 March 1995

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

Full work available at URL: https://doi.org/10.1063/1.530433

zbMATH Keywords

energy densityBirkhoff's theoremwallsVilenkin's planar wall

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) General relativity (83C99)

Related Items (2)

A class of plane symmetric dust solutions ⋮ A spin polarized disc. II

Cites Work

• Topological defects with axial symmetry: A disk + a string
• Isentropic Hydrodynamics in Plane Symmetric Space-Times
• The gravitational field of plane symmetric thick domain walls
• Exact self-gravitating disks and rings: A solitonic approach
• Self-similar relativistic discs with pressure
• Local stability of static self-similar relativistic discs against axisymmetric perturbations
• Topological defects: walls crossed by cosmic strings
• Topology of cosmic domains and strings
• Relativistic disks - I. Counter rotating disks
• Relativistic disks - II. Self-similar disks in rotation
• Formation of naked singularities: The violation of cosmic censorship
• On the Galactic Law of Rotation

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