“…For this reason in order to deal with finite energy weak solutions to (1.1), it is more convenient to consider the unknowns ( √ ρ, Λ), which define the hydrodynamic quantities by ρ = ( √ ρ) 2 , J = √ ρΛ, see Definition 15 below for more details. The lack of suitable a priori bounds prevents the study of solutions to (1.1) by using compactness arguments like it is done for viscous systems, see for example [8,7,51,58] where a viscous counterpart of system (1.1) is considered, see also [9,10] where a similar system is studied by using a suitable truncation argument. On the contrary, for the QHD system most of the existing results in the literature are perturbative [47,53,41,42].…”