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arXiv 2307.03151gr-qcastro-ph.HEhep-th
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稳态轴对称虫洞几何结构赤道面内的本轮频率

Epicyclic frequencies in the equatorial plane around stationary and axially symmetric wormhole geometries

Vittorio De Falco

AI总结:

本研究聚焦稳态轴对称虫洞赤道面内的本轮频率,提出区分虫洞与克尔黑洞的方法及利用观测数据重构虫洞度规的策略,为强引力场探测提供新的天体物理研究思路。

摘要:

本轮频率通常在X射线双星中被观测到,是探测致密天体周围强引力场的有力天体物理手段。我们研究了一般稳态轴对称虫洞周围赤道面内的本轮频率。我们首先探究虫洞的存在性,将其与克尔黑洞(Kerr black hole)区分开来。一旦获得虫洞的观测数据,我们提出了一种重构相关度规的策略。最后,我们讨论了该方法的意义并展望了未来可能的研究方向。

英文摘要:

Epicyclic frequencies are usually observed in X-ray binaries and constitute a powerful astrophysical mean to probe the strong gravitational field around a compact object. We consider them in the equatorial plane around a general stationary and axially symmetric wormhole. We first search for the wormholes' existence, distinguishing them from a Kerr black hole. Once there will be available observational data on wormholes, we present a strategy to reconstruct the related metrics. Finally, we discuss the implications of our approach and outline possible future perspectives.

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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