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On Preserving a B+L Asymmetry Produced in the Early Universe

Sacha Davidson, Hitoshi Murayama, Keith A. Olive

hep-pharXiv:hep-ph/9403259

Abstract

One of the most efficient mechanisms for producing the baryon asymmetry of the Universe is the decay of scalar condensates in a SUSY GUT as was first suggested by Affleck and Dine. We show that given a large enough asymmetry, the baryon number will be preserved down to low temperatures even if B - L = 0, because the baryon number carrying scalars form bose condensates that give the W a mass. We derive the conditions on the condensate needed to suppress electroweak sphaleron interactions which would otherwise drive the baryon asymmetry to zero when B - L = 0.

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