Renyi entropy and the topological features of charged AdS black hole

被引:0
作者
Yasir, Muhammad [1 ,2 ,3 ]
Tong, Lining [1 ,2 ]
Mushtaq, Farzan [1 ,2 ]
Xia, Tiecheng [1 ,2 ]
Upadhyay, Sudhaker [4 ,5 ,6 ,7 ]
Brzo, Aram Bahroz [8 ]
Pourhassan, Behnam [5 ,9 ,10 ]
机构
[1] Shanghai Univ, Dept Math, Shanghai 200444, Peoples R China
[2] Shanghai Univ, Newtouch Ctr Math, Shanghai 200444, Peoples R China
[3] ILMA Univ, Fac Sci & Technol, Dept Software Engn, Karachi 75190, Pakistan
[4] Magadh Univ, KLS Coll, Dept Phys, Bodh Gaya 805110, Bihar, India
[5] Damghan Univ, Sch Phys, POB 3671641167, Damghan, Iran
[6] LN Gumilyov Eurasian Natl Univ, Dept Gen & Theoret Phys, Astana 010008, Kazakhstan
[7] Canadian Quantum Res Ctr, 204-3002 32 Ave, Vernon, BC V1T 2L7, Canada
[8] Univ Sulaimani, Coll Educ, Phys Dept, Sulaimani 46001, Kurdistan Regio, Iraq
[9] Khazar Univ, Ctr Theoret Phys, 41 Mehseti St, AZ-1096 Baku, Azerbaijan
[10] Chitkara Univ, Ctr Res Impact & Outcome, Chitkara Univ Inst Engn & Technol, Rajpura 140401, Punjab, India
关键词
Black hole thermodynamics; Anti-de Sitter (AdS) spacetime; Thermodynamic topology; Modified gravity; THERMODYNAMICS;
D O I
10.1016/j.cjph.2025.03.022
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This study applies Duan's topological current phi-mapping theory to investigate a newly proposed charged modified AdS black hole using the R & eacute;nyi entropy formalism, examining thermodynamic properties across the canonical, mixed, and grand canonical ensembles. Electric and magnetic charges are fixed in the canonical ensemble, whereas the mixed ensemble incorporates electric and magnetic potentials. The grand canonical ensemble, meanwhile, ensures consistency by employing these potentials exclusively. Initially, we compute topological charges by identifying critical points in each ensemble. In both the canonical and mixed ensembles, we identify a conventional critical point with a topological charge of -1. We then model the black hole's domain in the AdS regime as a topological defect in thermodynamic space and analyze its local and global topology by calculating the winding numbers at these defect locations. Interestingly, the canonical and mixed ensembles exhibit identical black hole topologies, each possessing a total topological charge of 1 within the framework of the R & eacute;nyi entropy. Finally, we characterize the canonical, mixed, and grand canonical ensembles based on the presence of generation/annihilation points: the canonical ensemble has one such point, the mixed ensemble has a negative one, and the grand canonical ensemble has none.
引用
收藏
页码:1272 / 1288
页数:17
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