Scalar Field Condensate Baryogenesis Model in Different Inflationary
  Scenarios
  We calculate the baryon asymmetry value generated in the Scalar Field
Condensate (SCF) baryogenesis model obtained in several inflationary scenarios
and different reheating models. We provide analysis of the baryon asymmetry
value obtained for more than 70 sets of parameters of the SCF model and the
following inflationary scenarios, namely: new inflation, chaotic inflation,
Starobinsky inflation, MSSM inflation, quintessential inflation. We considered
both cases of efficient thermalization after inflation and also delayed
thermalization. We have found that SFC baryogenesis model produces baryon
asymmetry by orders of magnitude bigger than the observed one for the following
inflationary models: new inflation, new inflation model by Shafi and Vilenkin,
MSSM inflation, chaotic inflation with high reheating temperature and the
simplest Shafi-Vilenkin chaotic inflationary model. For these models strong
diluting mechanisms are needed to reduce the resultant baryon excess at low
energies to its observational value today. We have found that a successful
generation of the observed baryon asymmetry is possible by SCF baryogenesis
model in Modified Starobinsky inflation, chaotic inflation with low reheating
temperature, chaotic inflation in SUGRA and Quintessential inflation.
