Double cosmic walls in Teleparallel Gravity

dc.creatorde Andrade, L. C. Garcia
dc.date1999-08-27
dc.date.accessioned2026-07-07T03:33:31Z
dc.date.available2026-07-07T03:33:31Z
dc.descriptionAn example is given of a plane topological torsion defect representing a cosmic wall double wall in teleparallel gravity.The parallel planar walls undergone a repulsive gravitational force due to Cartan torsion.This is the first example of a non-Riemannian double cosmic wall.It is shown that the walls oscillate with a speed that depends on torsion and on the surface density of the wall.Cartan torsion acts also as a damping force reducing the speed of oscillation when it is stronger.
dc.descriptionLatex file 7 Kb
dc.identifierhttps://arxiv.org/abs/gr-qc/9908070
dc.identifierhttp://arxiv.org/abs/gr-qc/9908070
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36601
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleDouble cosmic walls in Teleparallel Gravity
dc.typetext

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