Quantum System under Periodic Perturbation: Effect of Environment

Abstract

In many physical situations the behavior of a quantum system is affected by interaction with a larger environment. We develop, using the method of influence functional, how to deduce the density matrix of the quantum system incorporating the effect of environment. After introducing characterization of the environment by spectral weight, we first devise schemes to approximate the spectral weight, and then a perturbation method in field theory models, in order to approximately describe the environment. All of these approximate models may be classified as extended Ohmic models of dissipation whose differences are in the high frequency part. The quantum system we deal with in the present work is a general class of harmonic oscillators with arbitrary time dependent frequency. The late time behavior of the system is well described by an approximation that employs a localized friction in the dissipative part of the correlation function appearing in the influence functional. The density matrix of the quantum system is then determined in terms of a single classical solution obtained with the time dependent frequency. With this one can compute the entropy, the energy distribution function, and other physical quantities of the system in a closed form. Specific application is made to the case of periodically varying frequency. This dynamical system has a remarkable property when the environmental interaction is switched off: Effect of the parametric resonance gives rise to an exponential growth of the populated number in higher excitation levels, or particle production in field theory models. The effect of the environment is investigated for this dynamical system and it is demonstrated that there exists

55 pages, LATEX file plus 13 PS figures. A few calculational mistatkes and corresponding figure 1 in field theory model corrected and some changes made for publication in Phys. Rev.D (in press)

References in corpus (13)

• Reheating after Inflation
• Universe Reheating after Inflation
• Classical decay of inflaton
• Non-Thermal Phase Transitions after Inflation
• Analytic and Numerical Study of Preheating Dynamics
• Reheating and Thermalization, Linear Vs. Non-Linear Relaxation
• The Universe after inflation: the wide resonance case
• Catastrophic Particle Production under Periodic Perturbation
• Particle Production and Dissipative Cosmic Field
• Reheating and thermalization in a simple scalar model
• Restriction to Parametric Resonant Decay after Inflation
• Baryogenesis and thermal history after inflation
• Decay Rate of Coherent Field Oscillation

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