Isotropy theorem for cosmological Yang-Mills theories

J. A. R. Cembranos, A. L. Maroto, and S. J. Núñez Jareño
Phys. Rev. D 87, 043523 – Published 13 February 2013

Abstract

We consider homogeneous non-Abelian vector fields with general potential terms in an expanding universe. We find a mechanical analogy with a system of N interacting particles (with N the dimension of the gauge group) moving in three dimensions under the action of a central potential. In the case of bounded and rapid evolution compared to the rate of expansion, we show by making use of a generalization of the virial theorem that for an arbitrary potential and polarization pattern, the average energy-momentum tensor is always diagonal and isotropic despite the intrinsic anisotropic evolution of the vector field. We consider also the case in which a gauge-fixing term is introduced in the action and show that the average equation of state does not depend on such a term. Finally, we extend the results to arbitrary background geometries and show that the average energy-momentum tensor of a rapidly evolving Yang-Mills field is always isotropic and has the perfect fluid form for any locally inertial observer.

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  • Received 21 December 2012

DOI:https://doi.org/10.1103/PhysRevD.87.043523

© 2013 American Physical Society

Authors & Affiliations

J. A. R. Cembranos, A. L. Maroto, and S. J. Núñez Jareño

  • Departamento de Física Teórica I, Universidad Complutense de Madrid, E-28040 Madrid, Spain

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Vol. 87, Iss. 4 — 15 February 2013

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