A new interior solution of Einstein's field equations for a spherically symmetric perfect fluid in shear-free motion

Statistics – Computation

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Computational Fluid Dynamics, Einstein Equations, Equations Of Motion, Field Theory (Physics), Ideal Fluids, Time Functions, Differential Equations, Flow Equations, Functional Integration, Shear Flow

Scientific paper

Although spherically symmetric expanding (or contracting) stars are a very important class of objects for the application of general relativity theory, only very few perfect solutions of Einstein's equations have been found so far. In this paper, a new class of exact solutions is presented which contains two arbitrary functions of time and one additional parameter.

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