How can the atomic orbital electrons be stable when moving through the epola?
The stability of the orbital electrons is given by the foundation of integer numbers of wavelengths of their accompanying epola deformation waves and the resulting electromagnetic waves (de Broglie waves). Having closed (elliptical) waveguides for the (absolute) motion of the electron protects the orbit from decay or excitation. Non-integer numbers of wavelengths per orbit will instantly decay by loss of energy to the epola. Two electrons are unable to share a waveguide path unless their spins are opposite – explaining the Pauli exclusion principle. When the atom is in motion through the epola, as it inevitably is, the waveguide can maintain its integrity by equally, on opposite sides of the orbit, losing and gaining random (thermal) eccentricities in the few from the billions of epola particles forming the waveguide when it distorts its ellipticity. In the case of hydrogen’s orbital electron, the electromagnetic waveguide is formed in accordance with Huygen’s rules, from secondary eff
