The use of relative quantum, RQ, functions to present a clear atomic model requires that the equations for quantum waveflow frequencies, wavelengths, and photon sizes be integrated into the relativistic time and mass transforms, with the mass to energy function: [ e = m (c^2) ]. This radiation of nuclear mass may be defined as a series of rates of nuclear change, [ dS/dt + d2S/dt2 + ... + dnS/dtn ]. Next, the psifunc may be written as a timespace integral for nucleoplastic pulsations of force particles. A model of this type uses quantized: space, time, probability, symmetry, magnetic, gravity, heat, charge, workons.
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The use of relative quantum, RQ, functions to present a clear atomic model requires that the equations for quantum waveflow frequencies, wavelengths, and photon sizes be integrated into the relativistic time and mass transforms, with the mass to energy function: [ e = m (c^2) ].
This radiation of nuclear mass may be defined as a series of rates of nuclear change, [ dS/dt + d2S/dt2 + ... + dnS/dtn ]. Next, the psifunc may be written as a timespace integral for nucleoplastic pulsations of force particles. A model of this type uses quantized: space, time, probability, symmetry, magnetic, gravity, heat, charge, workons.
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