ANISOTROPIC FLUIDS IN THE CASE OF STATIONARY AND AXISYMMETRIC SPACES OF GENERAL RELATIVITY

DOI10.1142/S0218271801001268zbMath1155.83317arXivgr-qc/0105012OpenAlexW3105300216MaRDI QIDQ3376521

Taxiarchis Papakostas

Publication date: 23 March 2006

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0105012

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (3)

GENERATING ANISOTROPIC FLUIDS FROM VACUUM ERNST EQUATIONS ⋮ Anisotropic magnetized sources in general relativity: An exact description for the magnetized vacuum ⋮ INTERIOR KERR SOLUTIONS WITH THE NEWMAN–JANIS ALGORITHM STARTING WITH STATIC PHYSICALLY REASONABLE SPACE–TIMES

Cites Work

• Riemannian-Maxwellian invertible structures in general relativity
• Anisotropic fluids and conformal motions in general relativity
• Confined gravitational fields produced by anisotropic fluids
• Hauser–Malhiot spaces admitting a perfect fluid energy-momentum tensor
• Orthogonal transitivity, invertibility, and null geodesic separability in type D electrovac solutions of Einstein’s field equations with cosmological constant
• The problem of exact interior solutions for rotating rigid bodies in general relativity
• New family of stationary and axisymmetric perfect-fluid solutions
• The Wahlquist metric cannot describe an isolated rotating body
• Stationary gravitational fields due to single bodies

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