Stability issues in the modified Starobinsky model

Abstract

We discuss the stability of the anomaly-induced inflation (modified Starobinsky model) with respect to the arbitrary choice of initial data and with respect to the small perturbations of the conformal factor and tensor modes of the metric in the later period of inflation and, partially, in the present Universe.

Talk presented at IRGA 2003 (Renormalization Group and Anomalies in Gravitation and Cosmology, Ouro Preto, Brazil, 16-23 March, 2003)

References in corpus (2)

• On the stability of the anomaly-induced inflation
• On the gravitational waves on the background of anomaly-induced inflation

Cited by in corpus (7)

• Effective Action of Vacuum: Semiclassical Approach
• From stable to unstable anomaly-induced inflation
• Effect of the Trace Anomaly on the Cosmological Constant
• On the scaling rules for the anomaly-induced effective action of metric and electromagnetic field
• One-loop renormalization of Lorentz/CPT violating scalar field theory in curved space-time
• Stochastic quantization of a self-interacting nonminimal scalar field in semiclassical gravity
• Bounce and stability in the early cosmology with anomaly-induced corrections