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- W2035702602 abstract "Using the Newman-Penrose spin-coefficient approach to gravitational radiation, we consider necessary conditions for stationary-radiative-stationary transitions to occur between states in a Riemannian space-time which satisfies the empty-space Einstein field equations everywhere outside of a spatially bounded timelike cylinder. It is found that for axially symmetric radiation of finite multipole expansion such transitions cannot occur; however, a model has been constructed for nonaxially symmetric radiation for which these transitions can occur to a certain asymptotic order in a relevant parameter while satisfying the Newman-Penrose conservation laws." @default.
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- W2035702602 title "Gravitational Radiation: Cutting the Tail" @default.
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- W2035702602 doi "https://doi.org/10.1063/1.1665172" @default.
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