Cosmological evolution in R^2 gravity
  The Universe evolution during the radiation-dominated epoch in the R^2-extended gravity theory is considered. The equations of motion for R and H are solved analytically and numerically. The particle production rate by the oscillating curvature is calculated in one-loop approximation and the back reaction of particle production on the evolution of R is taken into account. Possible implications of the model for cosmological creation of non-thermal dark matter is discussed. 
E. V. Arbuzova, A. D. Dolgov, L. Reverberi
gr-qc astro-ph.CO hep-ph