Thick domain walls coupled with viscous fluid and electromagnetic field in Lyra geometry
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Publication:1930030
DOI10.1007/s10773-012-1088-8zbMath1257.83028OpenAlexW2077623310MaRDI QIDQ1930030
V. R. Patil, D. D. Pawar, G. U. Khapekar
Publication date: 10 January 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1088-8
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)
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Cites Work
- Bianchi type-III cosmological models with time dependent displacement vector for barotropic fluid distribution in Lyra geometry
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- A static cosmological model in Einstein-Cartan theory
- Plane symmetric domain wall in Lyra geometry
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