Inflation in Einstein-Cartan theory with energy-momentum tensor with spin

Details Inflation in Einstein-Cartan theory with energy-momentum tensor with spin Inflation in Einstein-Cartan theory with energy-momentum tensor with spin

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phla..129..195f&link_type=abstract

Physics Letters A, Volume 129, Issue 4, p. 195-200.

Physics

9

Scientific paper

Generalized, or ``power-law'', inflation is shown to necessarily exist for a simple, anisotropic, (Bianchi type I) cosmology in the Einstein-Cartan gravitational theory with the Ray-Smalley improved energy-momentum tensor with spin. Formal solution of the EC field equations with the fluid equations of motion explicitly shows inflation caused by the RS spin angular kinetic energy density.

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