On a Non-Standard Atomic Model Developed in the Context of Bridge Electromagnetic Theory

The calculus of the orbital sommerfeld constant αn Let us consider an observer placed on a point P of an ideal expanding spherical surface ∑(t) inside which a dipole with fixed polarization in space and dipole moment d=eR is placed. The energy per unit time pertaining to an infinitesimal portion of the expanding surface is equal to the flux of the Poynting vector S of the source through the infinitesimal surface da. The total energy observed in P during the time interval t.