New Features about Chaos in Bianchi I non-Abelian Born-Infeld cosmology

Details New Features about Chaos in Bianchi I non-Abelian Born-Infeld cosmology New Features about Chaos in Bianchi I non-Abelian Born-Infeld cosmology

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..861..312d&link_type=abstract

ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP Conference Proceedings, Volume 861, pp. 312-319 (2006).

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Particle-Theory And Field-Theory Models Of The Early Universe, Gauge Field Theories, Strings And Branes

Scientific paper

When the action is replaced by the Born-Infeld-type non-Abelian action (NBI), a chaos-order transition is observed in the high energy region for a Bianchi I cosmology with the homogeneous SU(2) Yang-Mills field. This is interpreted as a smothering effect due to (non-perturbative in α') string corrections to the classical EYM action. We give a numerical evidence for the chaos-order transition and present an analytical proof of regularity of color oscillations in the limit of strong Born-Infeld non-linearity.

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