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  2. Schwinger–Dyson equation - Wikipedia

    en.wikipedia.org/wiki/SchwingerDyson_equation

    The Schwinger–Dyson equations (SDEs) or Dyson–Schwinger equations, named after Julian Schwinger and Freeman Dyson, are general relations between correlation functions in quantum field theories (QFTs).

  3. Feynman diagram - Wikipedia

    en.wikipedia.org/wiki/Feynman_diagram

    The technique of renormalization, suggested by Ernst Stueckelberg and Hans Bethe and implemented by Dyson, Feynman, Schwinger, and Tomonaga compensates for this effect and eliminates the troublesome infinities. After renormalization, calculations using Feynman diagrams match experimental results with very high accuracy.

  4. Dyson series - Wikipedia

    en.wikipedia.org/wiki/Dyson_series

    In scattering theory, a part of mathematical physics, the Dyson series, formulated by Freeman Dyson, is a perturbative expansion of the time evolution operator in the interaction picture. Each term can be represented by a sum of Feynman diagrams .

  5. Quantum electrodynamics - Wikipedia

    en.wikipedia.org/wiki/Quantum_electrodynamics

    Based on Bethe's intuition and fundamental papers on the subject by Shin'ichirō Tomonaga, [16] Julian Schwinger, [17] [18] Richard Feynman [1] [19] [20] and Freeman Dyson, [21] [22] it was finally possible to produce fully covariant formulations that were finite at any order in a perturbation series of quantum electrodynamics.

  6. Bethe–Salpeter equation - Wikipedia

    en.wikipedia.org/wiki/Bethe–Salpeter_equation

    The starting point for the derivation of the Bethe–Salpeter equation is the two-particle (or four point) Dyson equation = + in momentum space, where "G" is the two-particle Green function | | , "S" are the free propagators and "K" is an interaction kernel, which contains all possible interactions between the two particles.

  7. Interaction picture - Wikipedia

    en.wikipedia.org/wiki/Interaction_picture

    By utilizing the interaction picture, one can use time-dependent perturbation theory to find the effect of H 1,I, [15]: 355ff e.g., in the derivation of Fermi's golden rule, [15]: 359–363 or the Dyson series [15]: 355–357 in quantum field theory: in 1947, Shin'ichirō Tomonaga and Julian Schwinger appreciated that covariant perturbation ...

  8. History of quantum field theory - Wikipedia

    en.wikipedia.org/wiki/History_of_quantum_field...

    Quantum field theory originated in the 1920s from the problem of creating a quantum mechanical theory of the electromagnetic field.In particular, de Broglie in 1924 introduced the idea of a wave description of elementary systems in the following way: "we proceed in this work from the assumption of the existence of a certain periodic phenomenon of a yet to be determined character, which is to ...

  9. Schwinger's quantum action principle - Wikipedia

    en.wikipedia.org/wiki/Schwinger's_quantum_action...

    In Schwinger's approach, the action principle is targeted towards quantum mechanics. The action becomes a quantum action , i.e. an operator, S {\displaystyle S} . Although it is superficially different from the path integral formulation where the action is a classical function, the modern formulation of the two formalisms are identical.