|
|
Thermodynamic effects of Bardeen black hole surrounded by perfect fluid dark matter under general uncertainty principle |
Zhenxiong Nie(聂振雄), Yun Liu(刘芸), Juhua Chen(陈菊华)†, and Yongjiu Wang(王永久) |
Department of Physics, Key Laboratory of Low Dimensional Quantum Structures and Quantum Control of Ministry of Education, and Synergetic Innovation Center for Quantum Effects and Applications, Hunan Normal University, Changsha 410081, China |
|
|
Abstract The thermodynamics of Bardeen black hole surrounded by perfect fluid dark matter is investigated. We calculate the analytical expresses of corresponding thermodynamic variables, e.g., the Hawking temperature, entropy of the black hole. In addition, we derive the heat capacity to analyze the thermal stability of the black hole. We also compute the rate of emission in terms of photons through tunneling. By numerical method, an obvious phase transition behavior is found. Furthermore, according to the general uncertainty principle, we study the quantum corrections to these thermodynamic quantities and obtain the quantum-corrected entropy containing the logarithmic term. Lastly, we investigate the effects of the magnetic charge g, the dark matter parameter k and the generalized uncertainty principle parameter α on the thermodynamics of Bardeen black hole surrounded by perfect fluid dark matter under general uncertainty principle.
|
Received: 20 October 2021
Revised: 22 November 2021
Accepted manuscript online:
|
PACS:
|
04.60.Bc
|
(Phenomenology of quantum gravity)
|
|
04.70.Dy
|
(Quantum aspects of black holes, evaporation, thermodynamics)
|
|
Fund: This work was supported by the National Natural Science Foundation of China (Grant No.U1731107). |
Corresponding Authors:
Juhua Chen,E-mail:jhchen@hunnu.edu.cn
E-mail: jhchen@hunnu.edu.cn
|
About author: 2021-11-24 |
Cite this article:
Zhenxiong Nie(聂振雄), Yun Liu(刘芸), Juhua Chen(陈菊华), and Yongjiu Wang(王永久) Thermodynamic effects of Bardeen black hole surrounded by perfect fluid dark matter under general uncertainty principle 2022 Chin. Phys. B 31 050401
|
[1] Hawking S W 1975Commun. Math. Phys. 43 199 [2] Gibbons G W and Hawking S W 1977Phys. Rev. D 15 2738 [3] Sakalli I, Halilsoy M and Pasaoglu H 2012Astrophys. Space Sci. 340 155 [4] Kraus P and Wilczek F 1994Mod. Phys. Lett. A 9 3713 [5] Kraus P and Wilczek F 1995Nucl. Phys. B 437 231 [6] Parikh M K and Wilczek F 2000Phys. Rev. Lett. 85 5042 [7] Parikh M K 2002Phys. Lett. B 546 189 [8] Parikh M K 2004Int. J. Mod. Phys. D 13 2351 [9] Angheben M, Nadalini M, Vanzo L and Zerbini S 2005J. High Energy Phys. 2005(05) 014 [10] Srinivasan K and Padmanabhan T 1999Phys. Rev. D 60 024007 [11] Shankaranarayanan S, Srinivasan K and Padmanabhan T 2001Mod. Phys. Lett. 16 571 [12] Zhao R, Wu Y Q and Zhang L C 2003Class. Quantum Grav. 20 4885 [13] Sun X F and Wen B 2004Phys. Lett. A 19 677 [14] Kim Y W and Park Y J 2007Phys. Lett. B 655 172 [15] Yoon M, Ha J and Kim W 2007Phys. Rev. D 76 047501 [16] Nourcer K 2007Phys. Lett. B 646 63 [17] Anacieto M A, Brito F A, Passos E and Santos W P 2014Phys. Lett. B 737 6 [18] Anacieto M A, Brito F A and Passos E 2015Phys. Lett. B 749 181 [19] Kimura Y 2016Int. J. Mod. Phys. A 36 2150027 [20] Casini H, Huerta M and Myers R C 2011J. High Energy Phys. 2011(05) 036 [21] Wang J, Xu W and Meng X H 2014Phys. Rev. D 89 044034 [22] Magan J M, Melnikov D and Silva M R O 2014J. High Energy Phys. 2014(11) 069 [23] Majumder B 2013Gen. Rel. Grav. 45 2403 [24] Shen J, Liu C Z and Zhu N N 2019Acta Phys. Sin. 68 200401(in Chinese) [25] Kaul R K and Majumdar P 2000Phys. Rev. Lett. 84 5255 [26] Contreras E and Bargueno P 2018Mod. Phys. Lett. A 33 1850184 [27] Chen L S and Cheng H B 2017Int. J. Theor. Phys. 56 3572 [28] Feng Z W, Li H L, Zu X T and Yang S Z 2016Eur. Phys. J. C 76 212 [29] Carr B J, Mureika J and Nicolini P 2015J. High Energy Phys. 2015(07) 052 [30] Hawking S W and Ellis G F R 1973The large scale structure of space-time (Cambridge: Cambridge University Press) Vol. 1 [31] Hawking S W 1994 arXiv:9409195[hep-th] [32] Bardeen J M 1968Proceedings of the 5th Internationnal Conference on Gravitation and Relativity, August 16-17, 1968, Tbilisi, Georgia, p. 74 [33] Hayward S A 2006Phys. Rev. Lett. 96 031103 [34] Ayon-Beato E and Garcia A 1998Phys. Rev. Lett. 80 5056 [35] Berej W, Matyjasek J, Tryniecki D and Woronowicz M 2006Gen. Rel. Grav. 38 885 [36] Ade P A R et al. (Planck Collaboration) 2016Astron. Astrophys. 594 A23 [37] Kiselev V V 2003Class. Quantum Grav. 20 1187 [38] Toshmatov B, Stuchlík Z and Ahmedov B 2017Eur. Phys. J. P 132 98 [39] Benavides-Gallego C A, Abdujabbarov A and Bambi C 2020Phys. Rev. D 101 044038 [40] Kiselev V V 2020 arXiv:2003.0303031[gr-qc] [41] Gohar H and Saifullah K 2013 Astrophys. Space Sci. 343181 [42] Weinstein G 2021 arXiv:2102.11209[physics.hist-ph] [43] Bekenstein J D 1973Phys. Rev. D 7 2333 [44] Bekenstein J D 1974Phys. Rev. D 9 3292 [45] Hawking S W 1976Phys. Rev. D 13 191 [46] Maghsoodi E, Hassanabadi H and Chungb W S 2019 arXiv:1901.10305[gen-ph] [47] Lifshitz E M, Pitaevskii L P and Berestetskii V B 1982Quantum Electrodynamics (Oxford: Butterworth-Heinemann) [48] Camelia G A, Arzano M and Procaccini A 2020 arXiv:2004.0405084[gr-qc] [49] Ayon-Beato E and Garcia A 2000Phys. Lett. B 493 149 [50] Li M H and Yang K C 2012Phys. Rev. D 86 123015 [51] Zhang H X, Chen Y, He P Z, Fan Q Q and Deng J B 2020 arXiv:2007.09408[gr-qc] [52] Man J and Cheng H 2014Gen. Rel. Grav. 46 1660 [53] Emparan R 2000Phys. Rev. Lett. 85 499 [54] Taefik A 2013J. Cosmol. Astropart. Phys. 2013(07) 040 [55] Medved A J M and Vagenas E C 2004Phys. Rev. D 70 124021 |
No Suggested Reading articles found! |
|
|
Viewed |
|
|
|
Full text
|
|
|
|
|
Abstract
|
|
|
|
|
Cited |
|
|
|
|
Altmetric
|
blogs
Facebook pages
Wikipedia page
Google+ users
|
Online attention
Altmetric calculates a score based on the online attention an article receives. Each coloured thread in the circle represents a different type of online attention. The number in the centre is the Altmetric score. Social media and mainstream news media are the main sources that calculate the score. Reference managers such as Mendeley are also tracked but do not contribute to the score. Older articles often score higher because they have had more time to get noticed. To account for this, Altmetric has included the context data for other articles of a similar age.
View more on Altmetrics
|
|
|