General relativity with spin and torsion: Foundations and prospects

Friedrich W. Hehl, Paul von der Heyde, G. David Kerlick, and James M. Nester
Rev. Mod. Phys. 48, 393 – Published 1 July 1976
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Abstract

A generalization of Einstein's gravitational theory is discussed in which the spin of matter as well as its mass plays a dynamical role. The spin of matter couples to a non-Riemannian structure in space-time, Cartan's torsion tensor. The theory which emerges from taking this coupling into account, the U4 theory of gravitation, predicts, in addition to the usual infinite-range gravitational interaction medicated by the metric field, a new, very weak, spin contact interaction of gravitational origin. We summarize here all the available theoretical evidence that argues for admitting spin and torsion into a relativistic gravitational theory. Not least among this evidence is the demonstration that the U4 theory arises as a local gauge theory for the Poincaré group in space-time. The deviations of the U4 theory from standard general relativity are estimated, and the prospects for further theoretical development are assessed.

    DOI:https://doi.org/10.1103/RevModPhys.48.393

    ©1976 American Physical Society

    Authors & Affiliations

    Friedrich W. Hehl*, Paul von der Heyde, and G. David Kerlick

    • Institut für Theoretische Physik, Universität zu Köln, D-5000 Köln, 41, Federal Republic of Germany

    James M. Nester

    • Department of Physics and Astronomy, University of Maryland, College Park, Maryland 20742

    • *Supported by the Deutsche Forschungsgemeinschaft, Bonn.
    • Alexander von Humboldt Fellow.
    • Supported by NSF Grant GP43708X to the University of Maryland.

    See Also

    Gauge fields arising from spacetime symmetries and gravitational theories. I

    A. G. Agnese and P. Calvini
    Phys. Rev. D 12, 3800 (1975)

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    Issue

    Vol. 48, Iss. 3 — July - September 1976

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