Star-plus-wormhole systems with two interacting scalar fields
Vladimir Dzhunushaliev, Vladimir Folomeev, Ainur Urazalina
Abstract
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Vladimir Dzhunushaliev, Vladimir Folomeev, Ainur Urazalina
Abstract
Open-access reader
We study static, spherically symmetric mixed configurations with a nontrivial (wormhole) spacetime topology provided by the presence of two interacting ghost scalar fields. Wormhole is assumed to be filled by a perfect relativistic neutron fluid modeled by a polytropic equation of state. For such mixed configurations, we find regular, asymptotically flat general relativistic solutions. It is shown that the maximum of the fluid density is always shifted from the center and the resulting configurations represent, in general, double-throat systems.
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We study static, spherically symmetric mixed configurations with a nontrivial (wormhole) spacetime topology provided by the presence of two interacting ghost scalar fields. Wormhole is assumed to be filled by a perfect relativistic neutron fluid modeled by a polytropic equation of state. For such mixed configurations, we find regular, asymptotically flat general relativistic solutions. It is shown that the maximum of the fluid density is always shifted from the center and the resulting configurations represent, in general, double-throat systems.
Key concepts: Wormhole, Physics, Polytropic process, Scalar field, Equation of state, General relativity, Neutron star, Scalar (mathematics)