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Rotating wormhole solutions with a complex phantom scalar field

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arxiv 1906.08742 v1 pith:7LDCQBJ7 submitted 2019-06-20 gr-qc hep-th

classification gr-qchep-th
keywords solutionsfieldphantomcomplexrotatingscalarwormholeasymptotically
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We consider rotating wormhole solutions supported by a complex phantom scalar field with a quartic self-interaction, where the phantom field induces the rotation of the spacetime. The solutions are regular and asymptotically flat. A subset of solutions describing static but not spherically symmetric wormholes is also obtained.

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  1. Mass-Gap Neutron Stars from Vector \texorpdfstring{$f(R)$}{f(R)} Gravity Inflationary Deformations

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    Using four vector f(R) gravity inflation models and nine equations of state, the TOV solver finds that the MPA1 equation of state yields neutron star maximum masses around 2.75 solar masses, inside the mass gap.

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