从非扩展熵的角度看普遍关系

IF 5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Ankit Anand , Saeed Noori Gashti
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引用次数: 0

摘要

黑洞热力学的最新进展引入了修正来阐明熵与黑洞极值界之间的关系。传统上,这种关系是在以贝肯斯坦-霍金熵为特征的黑洞背景下研究的。然而,本研究将调查扩展到包含熵的非广泛概括。我们引入了一个小的常数修正,记为(j),并研究了带电反德西特(AdS)黑洞的普遍关系。我们的发现表明,当用熵的非广泛推广来描述带电AdS黑洞时,这些普遍关系并不成立。当然,经过一些调整,可以满足普适性关系。相反,当黑洞被贝肯斯坦-霍金熵描述时,宇宙关系仍然是相容的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Universal relations with the non-extensive entropy perspective
Recent advancements in black hole thermodynamics have introduced corrections to elucidate the relationship between entropy and extremality bound of black holes. Traditionally, this relationship has been studied in the context of black holes characterized by Bekenstein–Hawking entropy. However, this study extends the investigation to encompass non-extensive generalizations of entropy. We introduce a minor constant correction, denoted as (ɛ), and examine the universal relations for a charged Anti-de Sitter (AdS) black hole. Our findings indicate that these universal relations do not hold for the charged AdS black hole when described by the non-extensive generalizations of entropy. Of course, with some adjustments, the universality relations are met. In contrast, the universal relations remain compatible when the black hole is described by Bekenstein–Hawking entropy.
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来源期刊
Physics of the Dark Universe
Physics of the Dark Universe ASTRONOMY & ASTROPHYSICS-
CiteScore
9.60
自引率
7.30%
发文量
118
审稿时长
61 days
期刊介绍: Physics of the Dark Universe is an innovative online-only journal that offers rapid publication of peer-reviewed, original research articles considered of high scientific impact. The journal is focused on the understanding of Dark Matter, Dark Energy, Early Universe, gravitational waves and neutrinos, covering all theoretical, experimental and phenomenological aspects.
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