Local Structure of Numerically Generated Worm Hole Spacetime

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dc.creatorNambu, Yasusada
dc.creatorSiino, Masaru
dc.date1993-08-27
dc.date.accessioned2026-07-07T03:30:08Z
dc.date.available2026-07-07T03:30:08Z
dc.descriptionWe investigate the evolution of the apparent horizons in a numerically gererated worm hole spacetime. The behavior of the apparent horizons is affected by the dynamics of the matter field. By using the local mass of the system, we interpret the evolution of the worm hole structure. Figures are available by mail to author.
dc.description12pages
dc.identifierhttps://arxiv.org/abs/gr-qc/9308031
dc.identifierhttp://arxiv.org/abs/gr-qc/9308031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35437
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleLocal Structure of Numerically Generated Worm Hole Spacetime
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