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      Critical Parameterisation of the Brill Wave Initial Value Problem

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          Abstract

          A numerical framework to explore the Brill Wave Initial Value Problem is presented along with a review of some of the theoretical predictions concerning Brill waves. It is demonstrated that there is an agreement between the numerically observed phenomena and theory, namely that the IVP parameterisation of the metric function \(q\) has a minimum and maximum amplitude for which a solution to the Hamiltonian for the metric function \(\phi\) exists, and a critical regime in the middle for which there are and are not apparent horizons present.

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          On the positive definite mass of the Bondi-Weber-Wheeler time-symmetric gravitational waves

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            Author and article information

            Journal
            13 September 2018
            Article
            1809.05179
            041347bd-259f-4947-b7fd-06d2b5f59198

            http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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            Custom metadata
            8 pages, 8 figures
            gr-qc

            General relativity & Quantum cosmology
            General relativity & Quantum cosmology

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