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arXiv:hep-ph/9403259·v1·High Energy Physics — Phenomenology

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

Sacha Davidson🇺🇸 · Hitoshi Murayama🇺🇸 · Keith A. Olive🇺🇸

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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.

Comments: 10 pages, LaTeX, UMN-TH-1240, CfPA-TH-94-13, LBL-35275

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