Publication:
Field sources for Simpson-Visser spacetimes

dc.contributor.authorWalia, R. K.
dc.contributor.authorBronnikov, K. A.
dc.contributor.authorБронников, Кирилл Александрович
dc.date.accessioned2024-12-26T09:13:31Z
dc.date.available2024-12-26T09:13:31Z
dc.date.issued2022
dc.description.abstract© 2022 American Physical Society.Simpson-Visser (SV) spacetimes are the simplest globally regular modifications of the Schwarzschild, Reissner-Nordsröm and other black hole solutions of general relativity. They smoothly interpolate between these black holes and traversable wormholes. After a brief presentation of the Schwarzschild-like and Reissner-Nordsröm-like SV geometries, including their Carter-Penrose diagrams, we show that any static, spherically symmetric SV metric can be obtained as an exact solution to the Einstein field equations sourced by a combination of a minimally coupled phantom scalar field with a nonzero potential V(φ) and a magnetic field in the framework of nonlinear electrodynamics with the Lagrangian L(F), F=FμνFμν (in standard notations). Explicit forms of V(φ) and L(F) are presented for the cases of Schwarzschild-like and Reissner-Nordsröm-like SV metrics.
dc.identifier.citationWalia, R. K. Field sources for Simpson-Visser spacetimes / Walia, R.K., Bronnikov, K.A. // Physical Review D. - 2022. - 105. - № 4. - 10.1103/PhysRevD.105.044039
dc.identifier.doi10.1103/PhysRevD.105.044039
dc.identifier.urihttps://www.doi.org/10.1103/PhysRevD.105.044039
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dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/28812
dc.relation.ispartofPhysical Review D
dc.titleField sources for Simpson-Visser spacetimes
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume105
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