黑洞的 CR 体积和相应的熵变：综述

IF 11.7 2区物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS New Astronomy Reviews Pub Date : 2024-08-07 DOI:10.1016/j.newar.2024.101709

Shad Ali, Tong Liu

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引用次数: 0

摘要

本文回顾了有关黑洞内部体积、熵和蒸发的研究工作。本文介绍了理解黑洞内部体积的基础知识。本文解释了研究黑洞内部体积、相关量子模式熵以及内部和外部熵之间演化关系的一般类比。利用这一类比，我们预测了存储在黑洞中的信息、其辐射和蒸发的未来。结果见表 1 和表 2。为了将这一类比应用于 BH 时空，我们研究了不同类型 BH 的内部体积、熵和评价关系。最后，我们还研究了 BH 辐射的性质以及蒸发过程中粒子发射的概率。

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The CR volume for black holes and the corresponding entropy variation: A review

This paper reviews the work done on black hole interior volume, entropy, and evaporation. An insight into the basics for understanding the interior volume is presented. A general analogy to investigate the interior volume of a black hole, the associated quantum mode’s entropy, and the evolution relation between the interior and exterior entropy is explained. Using this analogy, we predicted the future of information stored in a BH, its radiation, and evaporation. The results are noted in tables 1 and 2. To apply this analogy in BH space–time, we investigated the interior volume, entropy, and evaluation relation for different types of BHs. Finally, we also investigated the nature of BH radiation and the probability of particle emission during the evaporation process.

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来源期刊

New Astronomy Reviews 地学天文-天文与天体物理

CiteScore

18.60

自引率

1.70%

发文量

审稿时长

11.3 weeks

期刊介绍： New Astronomy Reviews publishes review articles in all fields of astronomy and astrophysics: theoretical, observational and instrumental. This international review journal is written for a broad audience of professional astronomers and astrophysicists. The journal covers solar physics, planetary systems, stellar, galactic and extra-galactic astronomy and astrophysics, as well as cosmology. New Astronomy Reviews is also open for proposals covering interdisciplinary and emerging topics such as astrobiology, astroparticle physics, and astrochemistry.