Spinning fluids in general relativity. II. Self-consistent formulation

John R. Ray; Larry L. Smalley; Jean P. Krisch

doi:10.1103/PhysRevD.35.3261

Spinning fluids in general relativity. II. Self-consistent formulation

John R. Ray, Larry L. Smalley, and Jean P. Krisch

Phys. Rev. D 35, 3261 – Published 15 May 1987

Abstract

Methods used earlier to derive the equations of motion for a spinning fluid in the Einstein-Cartan theory are specialized to the case of general relativity. The main idea is to include the spin as a thermodynamic variable in the theory.

Received 12 November 1986

DOI:https://doi.org/10.1103/PhysRevD.35.3261

Authors & Affiliations

John R. Ray

Department of Physics and Astronomy, Clemson University, Clemson, South Carolina 29634-1911

Larry L. Smalley

ES65/Space Science Laboratory, Marshall Space Flight Center, Alabama 35812 and Department of Physics, University of Alabama in Huntsville, Huntsville, Alabama 35899

Jean P. Krisch

Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1120

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Vol. 35, Iss. 10 — 15 May 1987

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