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Black hole and wormhole solutions in Einstein-Maxwell-Scalar theory

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arxiv 2203.01278 v1 pith:4YJN4X2L submitted 2022-03-02 gr-qc astro-ph.HEhep-th

Black hole and wormhole solutions in Einstein-Maxwell-Scalar theory

classification gr-qc astro-ph.HEhep-th
keywords blackholeholeswormholeschargedfieldframepossible
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We classified and studied the charged black hole and wormhole solutions in the Einstein--Maxwell system in the presence of a massless, real scalar field. The possible existence of charged black holes in general scalar--tensor theories was studied in {Bronnikov et al, 1999;} black holes and wormholes exist for a negative kinetic term for the scalar field. Using a conformal transformation, the static, spherically symmetric possible structures in the minimal coupled system are described. Besides wormholes and naked singularities, only a restricted class of black hole exists, exhibiting a horizon with an infinite surface and a timelike central singularity. The black holes and wormholes defined in the Einstein frame have some specificities with respect to the non-minimal coupling original frame, which are discussed in the text.

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