Abstract
In the case of a spatially flat Friedmann--Lema\^ıtre--Robertson--Walker universe in -gravity we write the Wheeler-DeWitt equation of quantum cosmology. The equation depends on the functional form of . We select to work with four specific functions of , 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-Bäcklund transformations. In addition we show how the classical limit is recovered by the similarity solutions of the Wheeler-DeWitt equation.
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