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Abstract: We consider the evolution of cavities within spherically symmetricrelativistic fluids, under the assumption that proper radial distance betweenneighboring fluid elements remains constant during their evolution purelyareal evolution condition. The general formalism is deployed and solutions arepresented. Some of them satisfy Darmois conditions whereas others presentshells and must satisfy Israel conditions, on either one or both boundarysurfaces. Prospective applications of these results to some astrophysicalscenarios is suggested.



Author: L. Herrera, G. Le Denmat, N.O. Santos

Source: https://arxiv.org/



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