Rotating wormholes in Einstein-Dirac-Maxwell theory connect two flat spacetimes with different masses and charges, supported by spinor and electromagnetic fields and controlled by three input parameters.
Lawrie, A Unified Grand Tour of Theoretical Physics (Institute of Physics Publishing, Bristol, 2002)
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An asymmetric wormhole in Einstein-Dirac-Maxwell theory models a classical charged spinning particle with Standard Model mass and charge at one asymptotic end and Planck-scale values at the other.
An ad hoc source term added to the Dirac equation to model modified fermion anticommutation relations near black hole horizons produces stationary solutions interpreted as a fermion condensate.
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Rotating wormholes in Einstein-Dirac-Maxwell theory
Rotating wormholes in Einstein-Dirac-Maxwell theory connect two flat spacetimes with different masses and charges, supported by spinor and electromagnetic fields and controlled by three input parameters.
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Realistic classical charge from an asymmetric wormhole
An asymmetric wormhole in Einstein-Dirac-Maxwell theory models a classical charged spinning particle with Standard Model mass and charge at one asymptotic end and Planck-scale values at the other.
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Fermion condensate at the event horizon
An ad hoc source term added to the Dirac equation to model modified fermion anticommutation relations near black hole horizons produces stationary solutions interpreted as a fermion condensate.