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Quantum Fields

  • Philippe A. Martin
  • François Rothen
Part of the Texts and Monographs in Physics book series (TMP)

Abstract

In classical physics, a field is described by one or more space-time functions which satisfy certain partial differential equations. Several important examples were noted in Chap. 1: the vector potential A cl(x,t) of the electromagnetic field and the elastic displacement field u cl(x,t). One imagines a classical field as an infinite and continuous ensemble of degrees of freedom: a pair of dynamical variables is attached to each point x in space R 3, the amplitude u cl(x,t) of the field at time t and its time derivative (/∂t)u cl(x, t). The coupled evolution of this ensemble of degrees of freedom is governed by the differential equation of the field.

Keywords

Scalar Field Coherent State Gauge Field Canonical Variable Free Field 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2002

Authors and Affiliations

  • Philippe A. Martin
    • 1
  • François Rothen
    • 2
  1. 1.Institute for Theoretical PhysicsSwiss Federal Institute for TechnologyLausanneSwitzerland
  2. 2.Institute of Condensed Matter PhysicsUniversity of LausanneLausanneSwitzerland

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