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