Abstract:
In our conventional quantum theory, an electromagnetic potential plays two roles: it provides eigenstates for particles to be filled in and the particle eigenvalues. From the eigenvalues the potential provides the observed radiating energy. In mpm these two roles are separated. For a given quantum system, the energy radiated is captured from its surrounding super normal fluid. For an eigenstate in the nucleus, the gravitational interaction provides the place for a given nucleus while the electromagnetic interaction selects its appropriate angular Momentum, energy etc. of the chosen nucleon to fill in the place. The gravitational energy is too small to make any contribution for the radiation and the nucleons of the uncleus are protected with a very strong positive charge shell. When the matter-wave equation is Lorentz invariant it describes a nuclear bound state of the two potentials.