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Stability of charged thin shell wormhole supported by polytropic gas
Institution:1. Department of Physics, College of Science, Al Imam Mohammad Ibn Saud Islamic, University (IMSIU), Riyadh, KSA;2. Department of Astronomy, Faculty of Science, Cairo University, Giza, Egypt;1. Astronomy Dept., National Research Institute of Astronomy and Geophysics, (NRIAG), 11421, Box:138, Helwan, Cairo, Egypt.;2. Kottamia Center of Scientific Excellence in Astronomy and Space Sciences (KCScE) STDF, ASRT, Cairo, Egypt;1. Research Institute for Astronomy and Astrophysics of Maragha, Maragha, Iran;2. RIAAM Observatory, Research Institute for Astronomy and Astrophysics of Maragha, Maragha, Iran;1. National Research Institute of Astronomy and Geophysics, Astronomy Department, Helwan, Cairo, Egypt;2. Delaware State University, Dover, DE, USA
Abstract:In the framework of Darmois-Israel formalism, the general equations describing the motion of thin shell wormhole with a general form of equation of state of a polytropic gas are derived. The mechanical stability analysis of thin shell wormhole with charge in Reissner–Nordstrom (RN) to linearized spherically symmetric perturbation about static equilibrium solution is carried out.
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