Oscillation symmetry applied to some astrophysical masses, and allowing to highlight remarkable relations between masses

Abstract

The oscillation symmetry is applied to several exoplanet masses, quasars, binary neutron stars, and black holes in binary stellar systems. All studied data oscillate clearly and are well fitted with a simple cosine function. The same shape of mass oscillations is observed for different families, the masses of each familly being normalized by the same factor, showing a similarity between these shapes. Thus it is observed, for example, for a planet mass oscillation shape and fundamental particle mass oscillation shape, an oscillation period ratio between both