Thermodynamic topology of Hot NUT-Kerr-Newman-Kasuya-Anti-de Sitter black hole

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
M.U. Shahzad , Nazek Alessa , A. Mehmood , R. Javed
{"title":"Thermodynamic topology of Hot NUT-Kerr-Newman-Kasuya-Anti-de Sitter black hole","authors":"M.U. Shahzad ,&nbsp;Nazek Alessa ,&nbsp;A. Mehmood ,&nbsp;R. Javed","doi":"10.1016/j.ascom.2024.100900","DOIUrl":null,"url":null,"abstract":"<div><div>This work is devoted to studying the thermodynamic topology of Hot Nut-Kerr-Newman-Kasuya-AdS black holes (BHs). To accomplish this, we identify the critical points that play a crucial role in understanding the intricate structure of these BHs. We determine these critical points’ associated topological charges, providing important information about the underlying topology. Furthermore, we explore the concept of zero points and their corresponding winding numbers. These calculations allow us to evaluate the topological number associated with BHs and provide important information about their overall topological characteristics. One of the most important characteristics is the triple critical point. These points support the conjecture that the behavior of BHs undergoes significant transformations, presenting us with unique opportunities to observe and comprehend novel physical phenomena. A winding number of zero corresponds to a simple, connected horizon, while non-zero winding numbers indicate more complex topologies, such as multi-sheeted horizons. For comprehensive analysis, we fixed various parameters, such as the electric and magnetic charges and the electric and magnetic potentials. This approach allows us to isolate and examine specific aspects of BH topology.</div></div>","PeriodicalId":48757,"journal":{"name":"Astronomy and Computing","volume":"51 ","pages":"Article 100900"},"PeriodicalIF":1.9000,"publicationDate":"2024-12-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy and Computing","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S221313372400115X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

This work is devoted to studying the thermodynamic topology of Hot Nut-Kerr-Newman-Kasuya-AdS black holes (BHs). To accomplish this, we identify the critical points that play a crucial role in understanding the intricate structure of these BHs. We determine these critical points’ associated topological charges, providing important information about the underlying topology. Furthermore, we explore the concept of zero points and their corresponding winding numbers. These calculations allow us to evaluate the topological number associated with BHs and provide important information about their overall topological characteristics. One of the most important characteristics is the triple critical point. These points support the conjecture that the behavior of BHs undergoes significant transformations, presenting us with unique opportunities to observe and comprehend novel physical phenomena. A winding number of zero corresponds to a simple, connected horizon, while non-zero winding numbers indicate more complex topologies, such as multi-sheeted horizons. For comprehensive analysis, we fixed various parameters, such as the electric and magnetic charges and the electric and magnetic potentials. This approach allows us to isolate and examine specific aspects of BH topology.
热NUT-Kerr-Newman-Kasuya-Anti-de Sitter黑洞的热力学拓扑
本工作致力于热坚果-克尔-纽曼-卡舒亚- ads黑洞(BHs)的热力学拓扑研究。为了实现这一目标,我们确定了在理解这些黑洞的复杂结构中起关键作用的临界点。我们确定这些临界点的相关拓扑电荷,提供有关底层拓扑的重要信息。进一步探讨了零点的概念及其对应的圈数。这些计算使我们能够评估与黑洞相关的拓扑数,并提供有关其总体拓扑特征的重要信息。最重要的特征之一是三重临界点。这些观点支持这样一种猜想,即黑洞的行为经历了重大转变,为我们提供了观察和理解新的物理现象的独特机会。圈数为零对应于一个简单的、连通的视界,而非零的圈数表示更复杂的拓扑,如多层视界。为了综合分析,我们固定了各种参数,如电荷和磁荷以及电势和磁势。这种方法允许我们隔离和检查BH拓扑的特定方面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Astronomy and Computing
Astronomy and Computing ASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍: Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信