Abstract
The problem of charged perfect fluid and massive scalar field is investigated in the spacetime described by a general axially symmetric Jordan-Ehlers metric with two degrees of freedom. It is shown that the meson restmass $$\bar M$$ and the cosmological constant vanish, the electromagnetic field becomes source free and the perfect fluid degenerates to become a stiff perfect fluid (P=π). A class of exact solutions has been obtained removing one of the metric potentials. A method is also suggested to generate the most general solution. The physical behaviour and region of validity of the solutions are studied analytically.
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