Non-static conformally flat spherically symmetric space-times in Einstein-Cartan theory

DOI10.1016/J.CJPH.2019.03.010OpenAlexW2939308560WikidataQ128062371 ScholiaQ128062371MaRDI QIDQ6120236

L. N. Katkar, D. R. Phadatare

Publication date: 25 March 2024

Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cjph.2019.03.010

zbMATH Keywords

differential formskinematical parametersasymmetric connectionsCartan's equationsweyssenhoff fluid

Mathematics Subject Classification ID

General relativity (83Cxx) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83Dxx)

Related Items (1)

Static Weyssenhoff fluid sphere models in Einstein-Cartan theory of gravitation

Cites Work

• Static conformally flat spherically symmetric space-time in Einstein-Cartan theory of gravitation
• Non-static conformally flat spherically symmetric perfect fluid distribution in Einstein-Cartan theory
• A Newman-Penrose-type formalism for space-times with torsion
• A spin-coefficient approach to Weyssenhoff fluids in Einstein-Cartan theory
• An exact spherically symmetric space-time in Einstein-Cartan theory
• Einstein-Cartan theory of gravitation: kinematical parameters and Maxwell equations
• Lorentz Invariance and the Gravitational Field
• General relativity with spin and torsion: Foundations and prospects
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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