We propose the universal approach to describe spreading widths of monopole, dipole and quadrupole giant resonances in heavy and superheavy spherical nuclei. Our approach is based on the ideas of the random matrix distribution of the coupling between one-phonon and two-phonon states generated in the random phase approximation. We use the Skyrme interaction SLy4 as our model Hamiltonian to create a single-particle spectrum and to analyze excited states of the doubly magic nuclei 132 Sn, 208 Pb and 310 126. Our results demonstrate that the universal approach enables to describe gross structure of the spreading widths of the considered giant resonances. PACS numbers: 24.60.Lz, 21.60.Jz, 27.80.+w Damping of collective motion in finite many-body quantum systems is among topical subjects in mesoscopic physics. The question of how, for example, multipole giant resonances (GRs) in nuclei [1] and metal clusters [2] dissolve their energy is still not well understood. There is, however, a consensus of opinion that, in particular, in a nucleus, once excited by an external field, a GR progresses to a fully equilibrated system via direct particle emission and by coupling to more complicated states produced by the intrinsic motion of nucleons (see, for example, Ref.[3]). The former mechanism gives rise to escape width Γ p . It is expected that the decay evolution along the hierarchy of more complex configurations till compound states determines spreading width Γ. A full description of this decay represents a fundamental problem which is, however, difficult to solve (if even is possible at all ?) due to existence of many degrees of freedom.In general, the description of spreading width in mesoscopic systems is based on the study of the electromagnetic strength distribution (strength function) [4] in some energy interval. This interval should be large enough to catch hold of basic features of a GR under investigation. Note, that in deformed systems the experimental widths are systematically larger and may develop a two-or threepeak structure. In this paper we consider only spherical nuclei in order to highlight a generic nature of the width Γ in monopole, dipole and quadrupole resonances in heavy and super-heavy systems.Nuclear shell model may be used to analyse spreading widths of GRs. However, the complexity of the calculations increases rapidly with the size of the configuration space. This fact severely restricts the feasibility of shell model calculations for heavy and super-heavy nuclei. In addition, even for a medium 48 Ca isotope the state-of-art shell model calculations [5], which operate with the Hamiltonian matrices of a huge dimension, produce questionable results for the dipole GR. Although these calculations reproduce reasonably well its peak position and peak width, the enhancement of the classical Thomas-Reiche-Kuhn sum rules is too overestimated. As a result, the number of shell model studies, in particular, dipole GRs in heavy and super-heavy nuclei are limited and rather focused on details of low-energy regio...