Thin-shell wormholes in neo-Newtonian theory

Ali Övgün, Ines G. Salako

Resultado de la investigación: Contribución a una revistaArtículo de revisiónrevisión exhaustiva

6 Citas (Scopus)

Resumen

In this paper, we constructed an acoustic thin-shell wormhole (ATW) under neo-Newtonian theory using the Darmois-Israel junction conditions. To determine the stability of the ATW by applying the cut-and-paste method, we found the surface density and surface pressure of the ATW under neo-Newtonian hydrodynamics just after obtaining an analog acoustic neo-Newtonian solution. We focused on the effects of the neo-Newtonian parameters by performing stability analyses using different types of fluids, such as a linear barotropic fluid (LBF), a Chaplygin fluid (CF), a logarithmic fluid (LogF) and a polytropic fluid (PF). We showed that a fluid with negative energy is required at the throat to keep the wormhole stable. The ATW can be stable if suitable values of the neo-Newtonian parameters , A and B are chosen.

Idioma originalInglés
Número de artículo1750119
PublicaciónModern Physics Letters A
Volumen32
N.º23
DOI
EstadoPublicada - 30 jul. 2017
Publicado de forma externa

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