Realistic classical charge from an asymmetric wormhole
Vladimir Dzhunushaliev, Vladimir Folomeev
TL;DR
This work presents a classical mechanism to realize SM-scale mass and charge from a Planck-scale bare mass by coupling a complex spinor field and electromagnetic fields to gravity in an asymmetric, rotating wormhole setup. By solving the coupled Einstein-Dirac-Maxwell equations with a small throat and enforcing a one-particle normalization, the authors show that one wormhole end can exhibit masses and charges of SM particles while the other end remains at Planck scales. The configurations are inherently spinning, with total angular momentum obeying J = 1/2 Q_psi, and the gyromagnetic ratio g can differ significantly from the standard electron value, depending on throat size. This provides a classical analog of Wheeler’s ideas of ‘‘mass without mass’’ and ‘‘charge without charge’’ within a two-universe topology, highlighting a potential link between topology and observed particle properties.
Abstract
Within Einstein-Dirac-Maxwell theory, we consider a wormhole solution supported by a complex non-phantom spinor field with a bare mass of the order of the Planck mass (which provides a nontrivial spacetime topology and an intrinsic angular momentum), an electric field (which provides a charge of the system), and a magnetic field. This solution describes an asymmetric wormhole connecting two different asymptotically flat spacetimes (two universes) in which there are in general different observed masses and charges. It is shown that, by suitably adjusting the values of free system parameters, at one end of the wormhole, one can obtain the values of the observed mass and charge typical of the Standard Model particles, whereas at the other end of the wormhole these physical quantities acquire the Planck values. Such a configuration incarnates Wheeler's idea of ``mass without mass'' and ``charge without charge'', and can be thought of as a model of a classical charge possessing a spin.
