Gauge theories with time dependent couplings and their cosmological duals

Awad, Adel M.; Das, Sumit R.; Nampuri, Suresh; Narayan, K.; Trivedi, Sandip P.;

Abstract


We consider the N=4 super Yang-Mills theory in flat 3+1-dimensional space-time with a time dependent coupling constant which vanishes at t=0, like gYM2=tp. In an analogous quantum mechanics toy model we find that the response is singular. The energy diverges at t=0, for a generic state. In addition, if p>1 the phase of the wave function has a wildly oscillating behavior, which does not allow it to be continued past t=0. A similar effect would make the gauge theory singular as well, though nontrivial effects of renormalization could tame this singularity and allow a smooth continuation beyond t=0. The gravity dual in some cases is known to be a time dependent cosmology which exhibits a spacelike singularity at t=0. Our results, if applicable in the gauge theory for the case of the vanishing coupling, imply that the singularity is a genuine sickness and does not admit a meaningful continuation. When the coupling remains nonzero and becomes small at t=0, the curvature in the bulk becomes of order string scale. The gauge theory now admits a time evolution beyond this point. In this case, a finite amount of energy is produced which possibly thermalizes and leads to a black hole in the bulk. © 2009 The American Physical Society.


Other data

Title Gauge theories with time dependent couplings and their cosmological duals
Authors Awad, Adel M. ; Das, Sumit R.; Nampuri, Suresh; Narayan, K.; Trivedi, Sandip P.
Keywords High Energy Physics - Theory; High Energy Physics - Theory
Issue Date 2-Feb-2009
Journal Physical Review D - Particles, Fields, Gravitation and Cosmology 
Description 
45 pages, 1 figure; v2. minor modifications; v3: PRD version,
conclusions in the field theory case significantly revised to include
possible renormalization effects, quantum mechanics toy model unchanged,
abstract and introduction revised, additional subsection 4.1 added
ISSN 15507998
DOI 10.1103/PhysRevD.79.046004
Scopus ID 2-s2.0-61949363265

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