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 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.
Non-Abelian monopoles in modified gravity exhibit substantial structural and property differences from their Einstein-gravity counterparts, especially at strong Higgs self-coupling.
citing papers explorer
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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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Non-Abelian monopoles in modified gravity
Non-Abelian monopoles in modified gravity exhibit substantial structural and property differences from their Einstein-gravity counterparts, especially at strong Higgs self-coupling.