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arXiv 2309.17023gr-qc
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新型引力真空星解:在弦云与精质场存在下研究稳定性、能量与熵

Novel Gravastar Solutions: Investigating Stability, Energy, and Entropy in the Presence of Cloud of Strings and Quintessence

Faisal Javed, Ji Lin

AI总结:

本文在广义相对论框架下,将弦云与精质场引入Mazur-Mottola引力真空星模型,求解内外区域精确解并研究其稳定性、能量与熵,发现稳定性与弦云参数正相关、与精质场参数负相关。

摘要:

引力真空星(Gravastar)作为黑洞的理论替代天体,因其独特性质引起了天体物理学界的研究兴趣。本文旨在基于Mazur-Mottola(2004)方法,在广义相对论框架内进一步研究一种新型引力真空星模型的精确解,具体通过引入弦云(cloud of strings)和精质场(quintessence)来实现。通过分析引力真空星的引力场和能量密度,可以获得关于宇宙中致密天体本质的重要认识。理解引力真空星的稳定性对于我们认识黑洞及其他替代致密天体也至关重要。为此,我们给出了带有修正物质源的爱因斯坦场方程,并计算了引力真空星内部区域和中间区域的精确解。外部区域被视为由弦云和精质场包围的黑洞,并利用Darmoise-Israel形式体系对时空进行匹配。利用线性化径向微扰对引力真空星的稳定性进行了研究。此外,还计算了壳层的固有长度、能量含量和熵。引力真空星的稳定性与弦云参数的增强呈正相关,而与精质场参数的增长呈负相关。论文最后总结了研究发现及其在天体物理学和宇宙学领域的意义。

英文摘要:

Gravastars, theoretical alternatives to black holes, have captured the interest of scientists in astrophysics due to their unique properties. This paper aims to further investigate the exact solution of a novel gravastar model based on the Mazur-Mottola (2004) method within the framework of general relativity, specifically by incorporating the cloud of strings and quintessence. By analyzing the gravitational field and energy density of gravastars, valuable insights into the nature of compact objects in the universe can be gained. Understanding the stability of gravastars is also crucial for our comprehension of black holes and alternative compact objects. For this purpose, we present the Einstein field equations with the modified matter source and calculate the exact solutions for the inner and intermediate regions of gravastars. The exterior region is considered as a black hole surrounded by the cloud of strings and quintessence, and the spacetimes are matched using the Darmoise-Israel formalism. {An investigation is conducted on the stability of gravastars using linearized radial perturbation. Additionally, the proper length, energy content, and entropy of the shell are computed. The stability of gravastars is positively correlated with the enhancement of the cloud of strings parameter, while it is negatively correlated with the growth in the quintessence field parameter.} The paper concludes with a summary of the findings and their implications in the field of astrophysics and cosmology.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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