Thursday, December 22, 2011

1112.4995 (E. V. Arbuzova et al.)

Cosmological evolution in R^2 gravity    [PDF]

E. V. Arbuzova, A. D. Dolgov, L. Reverberi
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.
View original: http://arxiv.org/abs/1112.4995

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