Spherically symmetric Weitzenböck defect solution of Einstein field equation

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dc.creatorde Andrade, L. C. Garcia
dc.date2001-08-25
dc.date.accessioned2026-07-07T03:26:17Z
dc.date.available2026-07-07T03:26:17Z
dc.descriptionA new class of spacetime defect solutions of Einstein Field equations of Edelen's direct Poincaré Gauge Field theory without biaxial symmetry is presented. The interior solution describes a core of defects where curvature vanishes and Cartan torsion is nonvanishing. Outside the core (in vacuum) the solution represents a spacetime with vanishing curvature and torsion describing a nontrivial topological defect solution of Einstein equations of gravity. Our solution corresponds to a very weak strenght of Tachyons can be found far away from the core defect.
dc.descriptionLatex file
dc.identifierhttps://arxiv.org/abs/gr-qc/0108066
dc.identifierhttp://arxiv.org/abs/gr-qc/0108066
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33987
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSpherically symmetric Weitzenböck defect solution of Einstein field equation
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