Shear-free relativistic fluids and the absence of movable branch points

DOI10.1063/1.1455688zbMath1059.83009OpenAlexW2011408732MaRDI QIDQ4830780

Rodney G. Halburd

Publication date: 14 December 2004

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

Full work available at URL: https://semanticscholar.org/paper/c1ef30fc7655ac6bf2d0fe8e1eb7cfc76956cfb7

Mathematics Subject Classification ID

Painlevé and other special ordinary differential equations in the complex domain; classification, hierarchies (34M55) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (4)

On the meromorphic solutions of an equation of Hayman. ⋮ EVOLVING SPHERES OF SHEAR-FREE ANISOTROPIC FLUID ⋮ Painlevé Tests, Singularity Structure and Integrability ⋮ Charged sphere of shear-free fluids with \(\frac{\partial\rho}{\partial r} \leq 0\)

Cites Work

• Monodromy- and spectrum-preserving deformations. I
• Expanding spherically symmetric models without shear
• Solvable models of relativistic charged spherically symmetric fluids
• On spherically symmetric shear-free perfect fluid configurations (neutral and charged). I
• Jeffery-Williams Lecture, 1976 Non-Static Radially Symmetric Distributions of Matter

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