Constraints on Inflation in MSSM from Baryon Asymmetry

Details Constraints on Inflation in MSSM from Baryon Asymmetry Constraints on Inflation in MSSM from Baryon Asymmetry

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..805...17c&link_type=abstract

PARTICLES, STRINGS, AND COSMOLOGY: 11th International Symposium on Particles, Strings, and Cosmology; PASCOS 2005. AIP Conferen

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Particle-Theory And Field-Theory Models Of The Early Universe, Supersymmetric Models, Global Symmetries

Scientific paper

Finite density effects can change the inflationary reheating temperature of a large class of inflationary scenarios in the context of supersymmetry by a multiplicative factor of 1012. This gives the flat direction HuHd in MSSM a unique advantage over all other flat directions for being a participant in inflationary dynamics. More details concerning the content of this talk can be found in [1].

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