Causal perturbation theory

Causal perturbation theory is a mathematically rigorous approach to renormalization theory,[1] which makes it possible to put the theoretical setup of perturbative quantum field theory on a sound mathematical basis. It goes back to a seminal work by Henri Epstein and Vladimir Jurko Glaser.[2]


When developing quantum electrodynamics in the 1940s, Shin'ichiro Tomonaga, Julian Schwinger, Richard Feynman, and Freeman Dyson discovered that, in perturbative calculations, problems with divergent integrals abounded. The divergences appeared in calculations involving Feynman diagrams with closed loops of virtual particles. It is an important observation that in perturbative quantum field theory, time-ordered products of distributions arise in a natural way and may lead to ultraviolet divergences in the corresponding calculations. From the mathematical point of view, the problem of divergences is rooted in the fact that the theory of distributions is a purely linear theory, in the sense that the product of two distributions cannot consistently be defined (in general), as was proved by Laurent Schwartz in the 1950s.

Epstein and Glaser solved this problem for a special class of distributions that fulfill a causality condition, which itself is a basic requirement in axiomatic quantum field theory. In their original work, Epstein and Glaser studied only theories involving scalar (spinless) particles. Since then, the causal approach has been applied also to a wide range of gauge theories, which represent the most important quantum field theories in modern physics.


  1. Prange, Dirk (1 December 1998). "Epstein-Glaser renormalization and differential renormalization". Journal of Physics A: Mathematical and General. IOP Publishing. 32 (11): 2225–2238. arXiv:hep-th/9710225. doi:10.1088/0305-4470/32/11/015. ISSN 0305-4470.
  2. Epstein, H.; Glaser, V. (1973). "The role of locality in perturbation theory". Annales de l'Institut Henri Poincaré A. 29 (3): 211–295.

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