RT Journal Article
T1 Isotropy theorem for cosmological Yang-Mills theories
A1 López Maroto, Antonio
A1 Ruiz Cembranos, José Alberto
A1 Núñez Jareño, S. J.
AB 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.
PB American Physical Society
SN 1550-7998
YR 2013
FD 2013-02-13
LK https://hdl.handle.net/20.500.14352/33570
UL https://hdl.handle.net/20.500.14352/33570
LA eng
NO © 2013 American Physical Society.We thank Marco Peloso and Jose Beltrán Jiménez for useful comments. This work has been supported by MICINN (Spain) project numbers FIS2011-23000, FPA2011-27853-01, and Consolider-Ingenio MULTIDARK CSD2009-00064.
NO MICINN (Spain)
DS Docta Complutense
RD 10 abr 2025