Static fluid spheres in Einstein-Cartan theory

Details Static fluid spheres in Einstein-Cartan theory Static fluid spheres in Einstein-Cartan theory

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phrvd..11.2076p&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series, vol. 11, Apr. 15, 1975, p. 2076-2082.

Astronomy and Astrophysics

Astronomy

30

Astronomical Models, Einstein Equations, Ideal Fluids, Relativity, Space-Time Functions, Black Holes (Astronomy), Cosmology, Hydrostatic Pressure, Spheres

Scientific paper

The present work studies the Einstein-Cartan equations with special reference to a perfect fluid distribution. Three solutions are obtained by adopting Hehl's approach and Tolman's technique. It is found that a space-time metric similar to the Schwarzschild solution (interior) will no longer represent a homogeneous fluid sphere in the presence of spin density. At the boundary of the fluid sphere, the hydrostatic pressure is discontinuous.

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