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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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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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.