English

Expanding Spherically Symmetric Models without Shear

General Relativity and Quantum Cosmology 2009-10-28 v1

Abstract

The integrability properties of the field equation Lxx=F(x)L2L_{xx} = F(x)L^2 of a spherically symmetric shear--free fluid are investigated. A first integral, subject to an integrability condition on F(x)F(x), is found, giving a new class of solutions which contains the solutions of Stephani (1983) and Srivastava (1987) as special cases. The integrability condition on F(x)F(x) is reduced to a quadrature which is expressible in terms of elliptic integrals in general. There are three classes of solution and in general the solution of Lxx=F(x)L2L_{xx} = F(x)L^2 can only be written in parametric form. The case for which F=F(x)F=F(x) can be explicitly given corresponds to the solution of Stephani (1983). A Lie analysis of Lxx=F(x)L2L_{xx} = F(x) L^2 is also performed. If a constant α\alpha vanishes, then the solutions of Kustaanheimo and Qvist (1948) and of this paper are regained. For α0\alpha \neq 0 we reduce the problem to a simpler, autonomous equation. The applicability of the Painlev\'e analysis is also briefly considered.

Keywords

Cite

@article{arxiv.gr-qc/9511071,
  title  = {Expanding Spherically Symmetric Models without Shear},
  author = {Sunil D Maharaj and Peter GL Leach and Roy Maartens},
  journal= {arXiv preprint arXiv:gr-qc/9511071},
  year   = {2009}
}

Comments

14 pages LaTeX, to appear General Relativity and Gravitation