Gravitational torsion kinks and thick domain walls

dc.creatorde Andrade, L. C. Garcia
dc.date1998-11-13
dc.date.accessioned2026-07-25T17:19:08Z
dc.descriptionThe dynamics of a gravitational torsion kink as a plane symmetric thick domain wall solution of Einstein-Cartan (EC) field equation is given. The spin-torsion energy has to be as high as the gravitational kink potential otherwise torsion will not contribute as an appreciable effect to domain wall.Cartan torsion also contributes to the orthonal pressure of the domain wall.
dc.description5 pages latex
dc.identifierhttps://arxiv.org/abs/gr-qc/9811045
dc.identifierhttp://arxiv.org/abs/gr-qc/9811045
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/47567
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGravitational torsion kinks and thick domain walls
dc.typetext

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