General relativity with spin and torsion and its deviations from Einstein's theory

Friedrich W. Hehl, Paul von der Heyde, and G. David Kerlick
Phys. Rev. D 10, 1066 – Published 15 August 1974
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Abstract

The field equations of general relativity with spin and torsion (U4 theory) are considered to describe correctly the gravitational properties of matter on a microphysical level. By an averaging procedure one arrives at a macroscopic field equation, which under normal matter densities coincides with Einstein's equation of conventional general relativity. For very high matter densities, even if the spin are randomly distributed, Einstein's equation breaks down and U4 theory must be applied. It is shown how the singularity theorems of Penrose and Hawking must be modified to apply in U4 theory. All known cosmological models in U4 theory which prevent singularities are shown to violate an energy condition of a singularity theorem.

  • Received 29 April 1974

DOI:https://doi.org/10.1103/PhysRevD.10.1066

©1974 American Physical Society

Authors & Affiliations

Friedrich W. Hehl

  • Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08540

Paul von der Heyde

  • Institute for Theoretical Physics of the Technical University of Clausthal, 3392 Clausthal - Zellerfeld, West Germany

G. David Kerlick

  • Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08540

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Issue

Vol. 10, Iss. 4 — 15 August 1974

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