Thin-Shell Wormholes in Neo-Newtonian Theory
Thin-Shell Wormholes in Neo-Newtonian Theory
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DOI:
10.1142/s021773231750119x
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发表时间:
2017-02
期刊:
影响因子:
--
通讯作者:
A. Ovgun;I. G. Salako
中科院分区:
文献类型:
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作者:
A. Ovgun;I. G. Salako
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 $\varsigma$, $A$, and $B$ are chosen.