Published June 1998 | Version v1
Journal article

Asymptotic dynamics in scalar field theory: Anomalous relaxation

  • 1. Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260 (United States)
  • 2. Dipartimento di Fisica, Universita di Milano and INFN, Sezione di Milano, Via Celoria 16, 20133 Milano (Italy)
  • 3. LPTHE, Universite Pierre et Marie Curie (Paris VI) et Denis Diderot (Paris VII), Tour 16, 1er. etage, 4, Place Jussieu 75252 Paris, Cedex 05 (France)
  • 4. Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213 (United States)

Description

We analyze the dynamics of dissipation and relaxation in the unbroken and broken symmetry phases of scalar theory in the nonlinear regime for large initial energy densities, and after linear unstabilities (parametric or spinodal) are shut off by the quantum back reaction. A new time scale emerges that separates the linear from the non-linear regimes. This scale is non-perturbative in the coupling and initial amplitude. The non-perturbative evolution is studied within the context of the O(N) vector model in the large N limit. A combination of numerical analysis and the implementation of a dynamical renormalization group resummation via multi-time-scale analysis reveals the presence of unstable bands in the nonlinear regime. These are associated with power law growth of quantum fluctuations, that result in power law relaxation and dissipation with non-universal and non-perturbative dynamical anomalous exponents. We find that there is substantial particle production during this non-linear evolution which is of the same order as that in the linear regime and results in a non-perturbative distribution. The expectation value of the scalar field vanishes asymptotically transferring all of the initial energy into produced particles via the non-linear resonances in the unbroken symmetry phase. The effective mass squared for the quantum modes tends asymptotically to a constant plus oscillating O(1/t) terms. This slow approach to asymptotia causes the power behavior of the modes which become free harmonic modes for late enough time. We derive a simple expression for the equation of state for the fluid of produced particles that interpolates between radiation-type and dust-type equations according to the initial value of the order parameter for unbroken symmetry. For broken symmetry the produced particles are asymptotically massless Goldstone bosons with an ultrarelativistic equation of state. We find the onset of a novel form of dynamical Bose condensation in the collisionless regime in the absence of thermalization. copyright 1998 The American Physical Society

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
57
Journal Issue
12
Journal Page Range
p. 7388-7415
ISSN
0556-2821
CODEN
PRVDAQ