English

Non-Equilibrium Quantum Fields in the Large N Expansion

High Energy Physics - Phenomenology 2008-11-26 v1 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

An effective action technique for the time evolution of a closed system consisting of one or more mean fields interacting with their quantum fluctuations is presented. By marrying large NN expansion methods to the Schwinger-Keldysh closed time path (CTP) formulation of the quantum effective action, causality of the resulting equations of motion is ensured and a systematic, energy conserving and gauge invariant expansion about the quasi-classical mean field(s) in powers of 1/N1/N developed. The general method is exposed in two specific examples, O(N)O(N) symmetric scalar \l\F4\l\F^4 theory and Quantum Electrodynamics (QED) with NN fermion fields. The \l\F4\l\F^4 case is well suited to the numerical study of the real time dynamics of phase transitions characterized by a scalar order parameter. In QED the technique may be used to study the quantum non-equilibrium effects of pair creation in strong electric fields and the scattering and transport processes in a relativistic e+ee^+e^- plasma. A simple renormalization scheme that makes practical the numerical solution of the equations of motion of these and other field theories is described.

Keywords

Cite

@article{arxiv.hep-ph/9405352,
  title  = {Non-Equilibrium Quantum Fields in the Large N Expansion},
  author = {Fred Cooper and Salman Habib and Yuval Kluger and Emil Mottola and Juan Pablo Paz and Paul R. Anderson},
  journal= {arXiv preprint arXiv:hep-ph/9405352},
  year   = {2008}
}

Comments

43 pages, LA-UR-94-783 (PRD, in press), uuencoded PostScript

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