出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The anomaly-induced inflation (modi ed Starobinsky model) is based on the
application of the e
ective quantum eld theory approach to the Early Universe. We
present a brief general review of the model and show that it does not require a ne-tuning
for the parameters of the theory or initial data, gives a real chance to meet a graceful exit
to the FRW phase and also has positive features with respect to the metric perturbations.
