Study of Gravastar in Einstein-Gauss-Bonnet Gravity

IF 1.3 4区 物理与天体物理 Q3 PHYSICS, MULTIDISCIPLINARY
Hasrat Hussain Shah, Hassan Shah, Zahid Ahmad, Manel Hleili, Sardar Muhammad Hussain
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引用次数: 0

Abstract

The present work investigates a new model of the gravastar in a framework of 5-Dimensional (5D) Einstein-Gauss-Bonnet (EGB) gravitational theory. Adopting the approach of Mazur and Mottala (Proc. Natl. Acad. Sci., 101, 9545–9550, 2001, 2004) we divide the geometry of the stellar spherical object into three different portions, as follows (i) interior portion (ii) intermediate spherical thin shell and (iii) exterior portion. The interior portion contains dark energy having negative pressure. The thin shell region is made up of ultra-relativistic plasma where pressure and energy density are directly proportional. The exterior portion is completely vacuumed. By considering these assumptions, a set of stable and non-singular exact solutions for a gravastar has been investigated. In our model, graphical behavior shows that the obtained solution is physically reasonable and interesting.

爱因斯坦-高斯-波奈引力中的引力星研究
本研究在五维(5D)爱因斯坦-高斯-波奈(EGB)引力理论框架内研究了引力星的新模型。采用马祖尔和莫塔拉的方法(Proc. Natl.内部部分包含具有负压的暗能量。薄壳区域由超相对论等离子体组成,压力和能量密度成正比。外部部分是完全真空的。考虑到这些假设,我们研究了引力星的一组稳定且非奇异的精确解。在我们的模型中,图形行为表明所获得的解在物理上是合理和有趣的。
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来源期刊
CiteScore
2.50
自引率
21.40%
发文量
258
审稿时长
3.3 months
期刊介绍: International Journal of Theoretical Physics publishes original research and reviews in theoretical physics and neighboring fields. Dedicated to the unification of the latest physics research, this journal seeks to map the direction of future research by original work in traditional physics like general relativity, quantum theory with relativistic quantum field theory,as used in particle physics, and by fresh inquiry into quantum measurement theory, and other similarly fundamental areas, e.g. quantum geometry and quantum logic, etc.
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