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Computer algebra in gravity research. [PDF]
MacCallum MAH.
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Theorems on Existence and Global Dynamics for the Einstein Equations. [PDF]
Rendall AD.
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Expanding wave solutions of the Einstein equations that induce an anomalous acceleration into the Standard Model of Cosmology. [PDF]
Temple B, Smoller J.
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Static perfect fluid spacetimes on GRW spacetimes
Analysis and Mathematical Physics, 2023zbMATH Open Web Interface contents unavailable due to conflicting licenses.
De, Uday Chand, Sardar, Arpan
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Perfect fluid spacetimes and Yamabe solitons
Journal of Mathematical Physics, 2021This paper deals with the study of perfect fluid spacetimes. It is proven that a perfect fluid spacetime is Ricci recurrent if and only if the velocity vector field of perfect fluid spacetime is parallel and α = β. In addition, in a stiff matter perfect fluid Yang pure space with p + σ ≠ 0, the integral curves generated by the velocity vector field are
U. C. De, S. K. Chaubey, S. Shenawy
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Lanczos Potential and Perfect Fluid Spacetimes
International Journal of Theoretical Physics, 2011zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Ahsan, Zafar, Bilal, Mohd
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Investigation on gradient solitons in perfect fluid spacetimes
Reports on Mathematical Physics, 2023zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Krishnendu De, Uday Chand De
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Perfect fluid sources for spatially homogeneous spacetimes
Annals of Physics, 1983Abstract Spatially homogeneous perfect fluid spacetimes are studied from a point of view which emphasizes the spatial geometry and the action of that subgroup of the spatial gauge group of the three-plus-one formulation of general relativity which is compatible with the spatial homogeneity.
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Projective symmetry in perfect fluid spacetimes
Classical and Quantum Gravity, 2002Summary: Following a study of projective symmetry in Friedmann-Robertson-Walker models in \textit{G. S. Hall} [Classical Quantum Gravity 17, 4637-4644 (2000; Zbl 0988.83015)], it is shown (theorem 2) that the only conformally flat, perfect fluid spacetimes admitting such symmetry are, essentially, (locally) of the Friedmann-Robertson-Walker type.
Hall, G. S., Patel, M. T.
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