Electroweak Baryogenesis From Preheating After Inflation

Details Electroweak Baryogenesis From Preheating After Inflation Electroweak Baryogenesis From Preheating After Inflation

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.182g&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The explosive production of Higgs bosons at preheating in a low energy model of inflation may give rise to the required out of equilibrium state necessary for baryogenesis at the Electroweak scale. Diffusion at that stage ensures a large rate of sphaleron transitions, which may generate the observed baryon number of universe. This results are based on numerical simulations performed in (1+1)-dimensions.

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