Similarity solutions for the Wheeler-DeWitt equation in f( R) -cosmology

Abstract

In the case of a spatially flat Friedmann--Lema\tre--Robertson--Walker universe in f( R) -gravity we write the Wheeler-DeWitt equation of quantum cosmology. The equation depends on the functional form of f( R) . We select to work with four specific functions of f( R) , in which the field equations for the classical models are integrable and solvable through quadratures. For these models, we determine similarity solutions for the Wheeler-DeWitt equation by determine Lie-B\"acklund transformations. In addition we show how the classical limit is recovered by the similarity solutions of the Wheeler-DeWitt equation.

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