Bouncing Cosmology in f(Q) Symmetric Teleparallel Gravity
  We consider f(Q) extended symmetric teleparallel cosmologies, where Q is the
non-metricity scalar, and constrain its functional form through the order
reduction method. By using this technique, we are able to reduce and integrate
the field equations and thus to select the corresponding models giving rise to
bouncing cosmology. The selected Lagrangian is then used to develop the
Hamiltonian formalism and to obtain the Wave Function of the Universe which
suggests that classical observable universes can be recovered according to the
Hartle Criterion.
