Origin of hardening and universality of cosmic rays spectra in GV-PV
  rigidity region
  Recent balloon-borne and satellite experiments have established new features
in the behavior of the spectra of cosmic rays. An analysis of all the data
showed that hardening of most abundant primary cosmic ray nuclei spectra with
increasing rigidity is observed in $>200$ GV region. At the same time, rigidity
dependencies of secondary cosmic rays are distinctly different. The AMS-02 data
show that above 200 GV the secondary cosmic rays Li, Be, B harden more than the
primary He, C, O.
  In this paper we discuss a new scenario that self-consistently describes
these new features of the cosmic ray spectra. We demonstrate that the measured
by the AMS-02 changes in the slope of the cosmic ray spectra caused by the
transition from the contribution of multiple distant Galactic sources,
including the nuclear interactions of the particles accelerated by these
sources with an interstellar medium during their wandering in the Galaxy, to
the contribution of mainly local ones. We also found that the spectral
universality is observed at rigidity $R> 10^5$ GV.
