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2011

Cosmological evolution in R^2 gravity

Arbuzova, E. V., Dolgov, A. D., Reverberi, L.

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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.

Cosmological evolution in R^2 gravity · Around

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