“…The deformation of the external surface of the spherical shell with respect to the equilibrium sphere of the radius R can be represented through the multi pole expansion in spherical harmonics Y 1 m( t?, qJ), [l] The expansion coefficients a 1 m(t) are the dynamical variables that characterize the deformation. The orbital number I changes from 1=2 to ln==TCR.c/d (16) where dis a diameter of the particles constituting the globule, and m=-l, -1+ 1, ... l. The 1=0 mode is excluded by assumption that the volume of the globule is constant. The l= 1 Downloaded by [University of Connecticut] at 17:05 10 October 2014 mode is also excluded since it corresponds to the motion of the center of mass of the globule: it has been shown that such a motion practically does not affect the Mossbauer spectra (17,7,11).…”