We present a wormhole solution in four dimensions. It is a solution of an Einstein Maxwell theory plus charged massless fermions. The fermions give rise to a negative Casimir-like energy, which makes the wormhole possible. It is a long wormhole that does not lead to causality violations in the ambient space. It can be viewed as a pair of entangled near extremal black holes with an interaction term generated by the exchange of fermion fields. The solution can be embedded in the Standard Model by making its overall size small compared to the electroweak scale.
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Department of Physics and Astronomy, University of Victoria, Victoria, V8W 3P6, BCDepartment of Physics and Astronomy, University of Victoria, Victoria, V8W 3P6, BC
Harvey W.
Jensen K.
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Department of Physics and Astronomy, University of Victoria, Victoria, V8W 3P6, BCDepartment of Physics and Astronomy, University of Victoria, Victoria, V8W 3P6, BC
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UNIV WATERLOO,DEPT PHYS,GUELPH WATERLOO PROGRAM GRAD WORK PHYS,WATERLOO N2L 3G1,ONTARIO,CANADAUNIV WATERLOO,DEPT PHYS,GUELPH WATERLOO PROGRAM GRAD WORK PHYS,WATERLOO N2L 3G1,ONTARIO,CANADA
PERRY, GP
MANN, RB
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UNIV WATERLOO,DEPT PHYS,GUELPH WATERLOO PROGRAM GRAD WORK PHYS,WATERLOO N2L 3G1,ONTARIO,CANADAUNIV WATERLOO,DEPT PHYS,GUELPH WATERLOO PROGRAM GRAD WORK PHYS,WATERLOO N2L 3G1,ONTARIO,CANADA
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Univ Concepcion, Dept Fis, Casilla 160-C, Concepcion, ChileUniv Adolfo Ibanez, Dept Ciencias, Fac Artes Liberales, Ave Padre Hurtado 750, Vina Del Mar, Chile