Stationary cosmological solution with torsion

Details Stationary cosmological solution with torsion Stationary cosmological solution with torsion

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ncimb..87..101b&link_type=abstract

Nuovo Cimento B, Serie 11 (ISSN 0369-3554), vol. 87 B, June 11, 1985, p. 101-108. Research supported by the Conselho Nacional de

Mathematics

Logic

11

Cosmology, Gravitation Theory, Relativity, Rotating Fluids, Space-Time Functions, Unified Field Theory, Cartan Space, Density Distribution, Einstein Equations, Pressure Dependence, Torsion

Scientific paper

The role of torsion and spin has been studied in the case of stationary
universe with Weyssenhoff fluid under rigid rotation. It is shown that,
when the pressure bears a linear relation with the density, there exist
closed timelike lines. Only when the space-time is S - T homogeneous,
the spin can avoid closed timelike lines.

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