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Phys. Rev. D 72, 084021 (2005) [11 pages]

Chaos-order transition in Bianchi type I non-Abelian Born-Infeld cosmology

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Vladimir V. Dyadichev* and Dmitri V. Gal’tsov
Department of Theoretical Physics, Moscow State University, 119899, Moscow, Russia

Paulo Vargas Moniz‡,§
Astronomy Unit, School of Mathematical Sciences, University of London, Mile End Road, London E1 4NS, United Kingdom

Received 15 April 2005; published 24 October 2005

We investigate the Bianchi I cosmology with the homogeneous SU(2) Yang-Mills field governed by the non-Abelian Born-Infeld action. A similar system with the standard Einstein-Yang-Mills (EYM) action is known to exhibit chaotic behavior induced by the Yang-Mills field. When the action is replaced by the Born-Infeld–type non-Abelian action (NBI), the chaos-order transition is observed in the high-energy region. This is interpreted as a smothering effect due to (nonperturbative in α) string corrections to the classical EYM action. We give numerical evidence for the chaos-order transition and present an analytical proof of regularity of color oscillations in the limit of strong Born-Infeld nonlinearity. We also perform a general analysis of the Bianchi I NBI cosmology and derive an exact solution in the case of only the U(1) component excited. Our new exact solution generalizes the Rosen solution of the Bianchi I Einstein-Maxwell cosmology to the U(1) Einstein-Born-Infeld theory.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.72.084021
DOI:
10.1103/PhysRevD.72.084021
PACS:
04.20.Jb

*Electronic address: vv.dyadichev@pisem.net

Electronic address: galtsov@mail.phys.msu.ru

Electronic address: p.moniz@qmul.ac.uk

URL: http://webx.ubi.pt/~pmoniz

§On leave of absence from Departmento de Fisica, UBI, Covilha, Portugal.

Also at Centra-IST, Lisboa, Portugal.