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:
arXiv: General Relativity and Quantum Cosmology
影响因子:
--
通讯作者:
A. Ovgun;I. G. Salako
A. Ovgun;I. G. Salako
中科院分区:
其他
文献类型:
--
作者:
A. Ovgun;I. G. Salako

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在本文中,我们利用达穆瓦-以色列结条件在新牛顿理论下构造了声学薄壳虫洞(ATW)。为了通过应用剪切和粘贴方法确定 ATW 的稳定性,我们在获得模拟声学新牛顿解后立即找到了新牛顿流体动力学下 ATW 的表面密度和表面压力。我们通过使用不同类型的流体(例如线性正压流体 (LBF)、Chaplygin 流体 (CF)、对数流体 (LogF) 和多变流体 (PF))进行稳定性分析,重点关注新牛顿参数的影响。我们表明,喉部需要具有负能量的流体来保持虫洞的稳定。如果选择合适的新牛顿参数 $\varsigma$、$A$ 和 $B$ 值,ATW 可以稳定。
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.