Numerical Simulations of Electroweak Baryogenesis at Preheating

Details Numerical Simulations of Electroweak Baryogenesis at Preheating Numerical Simulations of Electroweak Baryogenesis at Preheating

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cosm.conf..355r&link_type=abstract

COSMO-2000 . Proceedings of the Fourth International Workshop on Particle Physics and the Early Universe . Held 4-8 September 20

Physics

Scientific paper

It has recently been suggested that the baryon washout problem of standard electroweak baryogenesis could be avoided if inflation ends at a low enough energy density and a parametric resonance transfers its energy repidly into the standard model fields. We present preliminary results of numerical simulations in a SU(2)×U(l) gauge-Higgs model in which this process was studied.

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