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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 families larger than 1055.

Keywords

oscillation symmetry, quantic families oscillate, kinetic energies, mass number

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