“…Note that UV finiteness does not mean that renormalisation is not needed at all: a finite renormalisation, with renormalisation constants depending on the Planck length, is needed, in order to subtract physically meaningless contributions; it should be possible to choose that dependence so that, applying this procedure to the usual renormalized interaction derived on the classical Minkowski space, the resulting perturbation expansion reproduces, in the limit λ P → 0, the usual renormalised perturbation expansion; however the interplay with the adiabatic limit and with the renormalised one particle states have to be considered; for progress on this line, see [75,76,77].…”