Classical aspects of weak interactions

Details Classical aspects of weak interactions Classical aspects of weak interactions

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hsei.conf....5k&link_type=abstract

Presented at the EPS Conference on Hadronic Structure and Electroweak Interactions, Amsterdam, Netherlands, 5-10 Aug. 1991

Physics

Classical Physics

Cosmology, Nuclear Models, Weak Interactions (Field Theory), Bosons, Fermions, Particle Collisions, Quantum Chromodynamics

Scientific paper

The classical physics of the electroweak standard model and its possible implications for cosmology and future particle collider experiments are discussed. It was seen that the classical field theory of electroweak interactions has an energy scale set by the sphaleron Es = O(Mw/alpha(weak)). Up till now small fluctuations around the vacuum at energies approximately alpha(weak)Es were probed. Under extreme conditions the nontrivial structure of configuration space may become important. An example of this may be anamalous B + h violation on an early epoch of the hot big bang. Whether or not similar conditions could be created in high energy particle colliders remains to be seen.

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