  This paper introduces novel solutions for inflation and late-time cosmic
acceleration within the framework of quantum Lovelock gravity, utilizing
Friedmann equations. Furthermore, we demonstrate the hypergeometric states of
cosmic acceleration through the Schr\"{o}dinger stationary equation. A physical
interpretation is proposed, whereby the rescaled Lovelock couplings represent a
topological mass that characterizes the Lovelock branch. This research holds
the potential for an extension into the quantum description. Predictions for
the spectral tilt and tensor-to-scalar ratio are depicted through plotted
curves. By utilizing the rescaled Hubble parameter, the spectral index is
determined in terms of the number of e-folds.
