Gravitational torsion kinks and thick domain walls

1998/11/13 by L. C. García de Andrade, L. C. Garcia de Andrade, de Andrade, L. C. Garcia
Physics and Astronomy · #Black Holes and Theoretical Physics #Nonlinear Photonic Systems #Nonlinear Waves and Solitons #gr-qc

paper · pdf · doi:10.48550/arxiv.gr-qc/9811045

5 pages latex

arxiv created 1998/11/13 · arxiv updated 2009/11/30

Abstract

The 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.

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