非对易施瓦西黑洞的热力学及其量子修正

沈珏; 刘成周; 朱宁宁; 童一诺; 严晨成; 薛珂磊

doi:10.7498/aps.68.20191054

摘要

为了探讨量子引力效应对黑洞量子性质的影响, 本文研究了非对易黑洞的热力学及其量子修正. 首先, 利用修正的黑洞热力学第一定律, 对非对易施瓦西黑洞的热力学量进行了计算. 结果表明, 利用修正的热力学第一定律得到的非对易黑洞温度与利用表面引力和隧穿方法得到的温度相同, 而且黑洞熵符合贝肯斯坦-霍金面积定律. 对得到的黑洞热容进行分析, 发现在视界半径与非对易参数满足一定条件时, 热容可以为正值, 非对易黑洞可以具有热力学稳定性. 其次, 讨论了广义不确定原理对非对易施瓦西黑洞热力学的影响, 给出了广义不确定原理修正的黑洞温度、熵和热容表达式, 其中得到的黑洞熵包含面积对数项. 在忽略广义不确定原理效应的情况下, 修正的黑洞熵可以回到贝肯斯坦-霍金面积定律的情况. 同样, 修正的黑洞温度和热容也可以在忽略量子引力效应时回到通常施瓦西黑洞的情况.

关键词:

Abstract

Black hole thermodynamics establishes a deep and satisfying link to gravity, thermodynamics, and quantum theory. And, the thermodynamic property of black hole is essentially a quantum feature of gravity. In this paper, in order to study the influence of the quantum gravity effect on the quantum properties of black hole, we study the thermodynamics and its quantum correction to a non-commutative black hole. First of all, the temperature of the non-commutative Schwarichild black hole is calculated by using three different methods: surface gravity, tunneling effects and the first law of black hole thermodynamics. It is found that the same hole temperature is obtained by means of the surface gravity and tunneling effects. However, by using the first law of black hole thermodynamics, different results are derived from the first two methods. Therefore, we incline to the result obtained by surface gravity and tunneling effects, and the temperature obtained by the thermodynamic law needs modifying. That is, for the non-commutative black hole, there is a contradiction to the first law of thermodynamics. To calculate the temperature and other thermodynamic quantities for the non-commutative Schwarichild black hole, we use the corrected first law of black hole thermodynamics proposed in the literature. It is found that the black hole temperature derived by the corrected first law is the same as the temperature obtained by the surface gravity and the tunneling model, and the black hole entropy still follows Beckenstein-Hawking area law. Also, the heat capacity of the black hole is obtained and analyzed. It is seen that when the horizon radius and non-commutative parameter satisfy the particular conditions, the heat capacity is positive and the non-commutative black holes are thermodynamically stable. This is a different result from that of the usual Schwarichild black hole. Further, by studying the influence of generalized uncertainty principle on non-commutative black hole thermodynamics, the quantum corrections from generalized uncertainty principle for temperature, entropy and heat capacity of the non-commutative Schwarzschild black hole are given. It is found that with considering this quantum gravity effect, the obtained black hole entropy contains the item of are alogarithm. If the effect of the generalized uncertainty principle is neglected, the corrected black hole entropy can return to that in the usual case of Beckenstein-Hawing area law. Similarly, the corrected black hole temperature and heat capacity can also return to their counterparts in the case of usual Schwarzschild black hole when this quantum gravity effect is ignored.

Keywords:

noncommutative black holes /
corrected first law of black hole thermodynamics /
generalize uncertainty principle /
quantum corrections

作者及机构信息

绍兴文理学院物理系, 绍兴　312000

通信作者: 刘成周, czlzj20@aliyun.com

基金项目: 浙江省自然科学基金(批准号: LY14A030001)和国家自然科学基金(批准号: 11373020)资助的课题

Authors and contacts

Department of Physics, Shaoxing University, Shaoxing 312000, China

Corresponding author: Liu Cheng-Zhou, czlzj20@aliyun.com

Funds: Project supported by the Natural Science Foundation of Zhejiang Pvovince, China (Grant No. LY14A030001) and the National Natural Science Foundation of China (Grant No. 11373020)

文章全文 : translate this paragraph

参考文献

[1]	Hawking S W 1974 Nature 248 30 Google Scholar
[2]	Hawking S W 1975 Commun. Math. Phys. 43 199 Google Scholar
[3]	Bekenstein J D 1973 Phys. Rev. D 7 2333
[4]	Wald R M 2001 Living Rev. Rel. 4 6 Google Scholar
[5]	蔡荣根, 曹利明 2016 科学通报 61 2083 Cai R G, Cao L M 2016 Chin. Sci. Bull. 61 2083
[6]	Garay L J 1995 Int. J. Mod. Phys. A 10 145 Google Scholar
[7]	Maggiore M 1993 Phys. Lett. B 304 65 Google Scholar
[8]	Kempf A, Mangano G, Mann R B 1995 Phys. Rev. D 52 1108 Google Scholar
[9]	Tawfik A, Diab A 2014 Int. J. Mod. Phys. D 23 1430025 Google Scholar
[10]	Chang L N, Minic D, Okamura N, Takeuchi T 2002 Phys. Rev. D 65 125028 Google Scholar
[11]	Li X 2002 Phys. Lett. B 540 9 Google Scholar
[12]	Liu C Z 2008 Sci. China Ser. G: Phys. Mech. Astron. 51 113 Google Scholar
[13]	Gangopadhyay S, Dutta A, Faizal M 2015 EPL 112 20006 Google Scholar
[14]	Li H L, Song D W, Li W 2019 Gen. Relat. Gravit. 51 20 Google Scholar
[15]	Chen D, Wu H, Yang H 2013 Adv. High. Energy Phys. 43 24126
[16]	Zhao R, Zhang S L 2006 Phys. Lett. B 641 318 Google Scholar
[17]	Majumder B 2011 Phys. Lett. B 703 402 Google Scholar
[18]	Banerjee R, Ghosh S 2010 Phys. Lett. B 688 224 Google Scholar
[19]	Medved A J M, Vagenas E C 2004 Phys. Rev. D 70 124021 Google Scholar
[20]	Anacleto M A, Brito F A, Passos E 2015 Phys. Lett. B 749 181 Google Scholar
[21]	Yoon M, Ha J, Kim W 2007 Phys. Rev. D 76 047501 Google Scholar
[22]	Anacleto M A, Bazeia D, Brito F A, Mota-Silva J C 2016 Adv. High. Energy Phys. 11 8465759
[23]	Maluf R V, Neves J C S 2018 Phys. Rev. D 97 104015 Google Scholar
[24]	Casadio R, Nicolini P, da Rocha R 2018 Class. Quant. Grav. 35 185001 Google Scholar
[25]	Myung Y S, Kim Y W, Park Y J 2007 Phys. Lett. B 645 393 Google Scholar
[26]	Witten E 1996 Nucl. Phys. B 460 335 Google Scholar
[27]	Szabo R J 2003 Phys. Rept. 378 207 Google Scholar
[28]	Nasseri F 2005 Gen. Relat. Gravit. 37 2223 Google Scholar
[29]	Nicolini P, Smailagic A, Spallucci E 2006 Phys. Lett. B 632 547 Google Scholar
[30]	Lopez-Dominguez J C, Obregon O, Sabido M, Ramirez C 2006 Phys. Rev. D 74 084024 Google Scholar
[31]	Chaichian M, Tureanu A, Zet G 2008 Phys. Lett. B 660 573 Google Scholar
[32]	Kobakhidze A 2009 Phys. Rev. D 79 047701 Google Scholar
[33]	Nicolini P 2005 J. Phys. A 38 L631 Google Scholar
[34]	Gruppuso A 2005 J. Phys. A 38 2039 Google Scholar
[35]	Cai R G, Wang A 2010 Phys. Lett. B 686 166 Google Scholar
[36]	Nicolini P, Smailagic A, Spallucci E 2006 ESA Spec. Publ. 637 547
[37]	Nozari K, Fazlpour B 2007 Mod. Phys. Lett. A 22 2917 Google Scholar
[38]	Banerjee R, Majhi B R, Samanta S 2008 Phys. Rev. D 77 124035 Google Scholar
[39]	Baneriee R, Majhi B R, Modak S K 2009 Class. Quant. Grav. 26 085010 Google Scholar
[40]	Nozari K, Mehdipour S H 2008 Class. Quant. Grav. 25 175015 Google Scholar
[41]	Myung Y S, Kim Y W, Park Y J 2007 JHEP 0702 012
[42]	Kim W, Son Edwin J, Yoon M 2008 JHEP 0804 042
[43]	Vakili B, Khosravi N, Sepangi H R 2009 Int. J. Mod. Phys. D 18 159 Google Scholar
[44]	Buric M, Madore J 2008 Eur. Phys. J. C 58 347 Google Scholar
[45]	Huang W H, Huang K W 2009 Phys. Lett. B 670 416 Google Scholar
[46]	Nozari K, Mehdipour S H 2009 JHEP 0903 061
[47]	Nozari K, Islamzadeh S 2013 Astrophys. Space. Sci. 347 299 Google Scholar
[48]	Mehdipour S H, Keshavarz A 2012 Europhys. Lett. 9 10002
[49]	Sharif M, Javed W 2011 Can. J. Phys. 89 1027 Google Scholar
[50]	Faizal M, Amorim R G G, Ulhoa S C 2015 Int. J. Mod. Phys. D 27 1850053
[51]	Ma M S, Zhao R 2014 Class. Quantum. Grav. 31 24
[52]	Casadio R, Micu O, Nicolini P 2015 High. Energy Phys. 178 293
[53]	Ali A F, Nafie H, Shalaby M 2012 Europhys. Lett. 100 20004 Google Scholar
[54]	Liu Z Y, Ren J R 2014 Commun. Theor. Phys. 62 819 Google Scholar
[55]	Mu B, Wang P, Yang H 2015 Adv. High. Energy Phys. 2015 1
[56]	Ma H, Li J 2017 Chin. Phys. B 26 60401 Google Scholar
[57]	Chen N S, Zhang J Y 2015 Chin. Phys. B 24 020401 Google Scholar
[58]	Ibungochouba S T 2015 Chin. Phys. B 24 70401 Google Scholar
[59]	Ye B B, Chen J H, Wang Y J 2017 Chin. Phys. B 26 90202 Google Scholar
[60]	刘成周, 邓岳君, 骆叶成 2018 物理学报 67 060401 Google Scholar Liu C Z, Deng Y J, Luo Y C 2018 Acta Phys. Sin. 67 060401 Google Scholar
[61]	吴迪, 朱晓丹, 吴双清 2014 物理学报 63 180401 Google Scholar Wu D, Zhu X D, Wu S Q 2014 Acta Phys. Sin. 63 180401 Google Scholar
[62]	Parikh M K, Wilczek F 2000 Phys. Rev. Lett. 85 5042 Google Scholar
[63]	Parikh M K 2004 Int. J. Mod. Phys. D 13 2351 Google Scholar
[64]	Painleve P 1921 C. R. Acad. Sci. (Paris) 173 677
[65]	刘辽, 赵峥 2004 广义相对论(北京: 高等教育出版社) 第109页 Liu L, Zhao Z 2004 General Relativity (Beijing: Higher Education Press) p109 (in Chinese)
[66]	Camellia G A, Arzano M, Procaccini A 2014 Phys. Rev. D 70 107501

施引文献

[1]	Hawking S W 1974 Nature 248 30 Google Scholar
[2]	Hawking S W 1975 Commun. Math. Phys. 43 199 Google Scholar
[3]	Bekenstein J D 1973 Phys. Rev. D 7 2333
[4]	Wald R M 2001 Living Rev. Rel. 4 6 Google Scholar
[5]	蔡荣根, 曹利明 2016 科学通报 61 2083 Cai R G, Cao L M 2016 Chin. Sci. Bull. 61 2083
[6]	Garay L J 1995 Int. J. Mod. Phys. A 10 145 Google Scholar
[7]	Maggiore M 1993 Phys. Lett. B 304 65 Google Scholar
[8]	Kempf A, Mangano G, Mann R B 1995 Phys. Rev. D 52 1108 Google Scholar
[9]	Tawfik A, Diab A 2014 Int. J. Mod. Phys. D 23 1430025 Google Scholar
[10]	Chang L N, Minic D, Okamura N, Takeuchi T 2002 Phys. Rev. D 65 125028 Google Scholar
[11]	Li X 2002 Phys. Lett. B 540 9 Google Scholar
[12]	Liu C Z 2008 Sci. China Ser. G: Phys. Mech. Astron. 51 113 Google Scholar
[13]	Gangopadhyay S, Dutta A, Faizal M 2015 EPL 112 20006 Google Scholar
[14]	Li H L, Song D W, Li W 2019 Gen. Relat. Gravit. 51 20 Google Scholar
[15]	Chen D, Wu H, Yang H 2013 Adv. High. Energy Phys. 43 24126
[16]	Zhao R, Zhang S L 2006 Phys. Lett. B 641 318 Google Scholar
[17]	Majumder B 2011 Phys. Lett. B 703 402 Google Scholar
[18]	Banerjee R, Ghosh S 2010 Phys. Lett. B 688 224 Google Scholar
[19]	Medved A J M, Vagenas E C 2004 Phys. Rev. D 70 124021 Google Scholar
[20]	Anacleto M A, Brito F A, Passos E 2015 Phys. Lett. B 749 181 Google Scholar
[21]	Yoon M, Ha J, Kim W 2007 Phys. Rev. D 76 047501 Google Scholar
[22]	Anacleto M A, Bazeia D, Brito F A, Mota-Silva J C 2016 Adv. High. Energy Phys. 11 8465759
[23]	Maluf R V, Neves J C S 2018 Phys. Rev. D 97 104015 Google Scholar
[24]	Casadio R, Nicolini P, da Rocha R 2018 Class. Quant. Grav. 35 185001 Google Scholar
[25]	Myung Y S, Kim Y W, Park Y J 2007 Phys. Lett. B 645 393 Google Scholar
[26]	Witten E 1996 Nucl. Phys. B 460 335 Google Scholar
[27]	Szabo R J 2003 Phys. Rept. 378 207 Google Scholar
[28]	Nasseri F 2005 Gen. Relat. Gravit. 37 2223 Google Scholar
[29]	Nicolini P, Smailagic A, Spallucci E 2006 Phys. Lett. B 632 547 Google Scholar
[30]	Lopez-Dominguez J C, Obregon O, Sabido M, Ramirez C 2006 Phys. Rev. D 74 084024 Google Scholar
[31]	Chaichian M, Tureanu A, Zet G 2008 Phys. Lett. B 660 573 Google Scholar
[32]	Kobakhidze A 2009 Phys. Rev. D 79 047701 Google Scholar
[33]	Nicolini P 2005 J. Phys. A 38 L631 Google Scholar
[34]	Gruppuso A 2005 J. Phys. A 38 2039 Google Scholar
[35]	Cai R G, Wang A 2010 Phys. Lett. B 686 166 Google Scholar
[36]	Nicolini P, Smailagic A, Spallucci E 2006 ESA Spec. Publ. 637 547
[37]	Nozari K, Fazlpour B 2007 Mod. Phys. Lett. A 22 2917 Google Scholar
[38]	Banerjee R, Majhi B R, Samanta S 2008 Phys. Rev. D 77 124035 Google Scholar
[39]	Baneriee R, Majhi B R, Modak S K 2009 Class. Quant. Grav. 26 085010 Google Scholar
[40]	Nozari K, Mehdipour S H 2008 Class. Quant. Grav. 25 175015 Google Scholar
[41]	Myung Y S, Kim Y W, Park Y J 2007 JHEP 0702 012
[42]	Kim W, Son Edwin J, Yoon M 2008 JHEP 0804 042
[43]	Vakili B, Khosravi N, Sepangi H R 2009 Int. J. Mod. Phys. D 18 159 Google Scholar
[44]	Buric M, Madore J 2008 Eur. Phys. J. C 58 347 Google Scholar
[45]	Huang W H, Huang K W 2009 Phys. Lett. B 670 416 Google Scholar
[46]	Nozari K, Mehdipour S H 2009 JHEP 0903 061
[47]	Nozari K, Islamzadeh S 2013 Astrophys. Space. Sci. 347 299 Google Scholar
[48]	Mehdipour S H, Keshavarz A 2012 Europhys. Lett. 9 10002
[49]	Sharif M, Javed W 2011 Can. J. Phys. 89 1027 Google Scholar
[50]	Faizal M, Amorim R G G, Ulhoa S C 2015 Int. J. Mod. Phys. D 27 1850053
[51]	Ma M S, Zhao R 2014 Class. Quantum. Grav. 31 24
[52]	Casadio R, Micu O, Nicolini P 2015 High. Energy Phys. 178 293
[53]	Ali A F, Nafie H, Shalaby M 2012 Europhys. Lett. 100 20004 Google Scholar
[54]	Liu Z Y, Ren J R 2014 Commun. Theor. Phys. 62 819 Google Scholar
[55]	Mu B, Wang P, Yang H 2015 Adv. High. Energy Phys. 2015 1
[56]	Ma H, Li J 2017 Chin. Phys. B 26 60401 Google Scholar
[57]	Chen N S, Zhang J Y 2015 Chin. Phys. B 24 020401 Google Scholar
[58]	Ibungochouba S T 2015 Chin. Phys. B 24 70401 Google Scholar
[59]	Ye B B, Chen J H, Wang Y J 2017 Chin. Phys. B 26 90202 Google Scholar
[60]	刘成周, 邓岳君, 骆叶成 2018 物理学报 67 060401 Google Scholar Liu C Z, Deng Y J, Luo Y C 2018 Acta Phys. Sin. 67 060401 Google Scholar
[61]	吴迪, 朱晓丹, 吴双清 2014 物理学报 63 180401 Google Scholar Wu D, Zhu X D, Wu S Q 2014 Acta Phys. Sin. 63 180401 Google Scholar
[62]	Parikh M K, Wilczek F 2000 Phys. Rev. Lett. 85 5042 Google Scholar
[63]	Parikh M K 2004 Int. J. Mod. Phys. D 13 2351 Google Scholar
[64]	Painleve P 1921 C. R. Acad. Sci. (Paris) 173 677
[65]	刘辽, 赵峥 2004 广义相对论(北京: 高等教育出版社) 第109页 Liu L, Zhao Z 2004 General Relativity (Beijing: Higher Education Press) p109 (in Chinese)
[66]	Camellia G A, Arzano M, Procaccini A 2014 Phys. Rev. D 70 107501

[1]	米尔阿里木江, 艾力, 买买提热夏提, 买买提, 亚森江, 吾甫尔. 非对易相空间中谐振子体系热力学性质的探讨. 物理学报, 2015, 64(14): 140201. doi: 10.7498/aps.64.140201
[2]	李鹤龄, 王娟娟, 杨斌, 王亚妮, 沈宏君. 广义不确定性原理下费米气体低温热力学性质. 物理学报, 2015, 64(8): 080502. doi: 10.7498/aps.64.080502
[3]	郑伯昱, 董慧龙, 陈非凡. 基于量子修正的石墨烯纳米带热导率分子动力学表征方法. 物理学报, 2014, 63(7): 076501. doi: 10.7498/aps.63.076501
[4]	邓玮, 方洁, 吴振军, 吴艳敏. 含有不确定项的混沌系统自适应修正函数投影同步. 物理学报, 2012, 61(14): 140503. doi: 10.7498/aps.61.140503
[5]	黄海, 贺锋, 孙航宾. 利用广义不确定关系计算 Reissner-Nordstrm-de Sitter黑洞的统计力学熵. 物理学报, 2012, 61(11): 110403. doi: 10.7498/aps.61.110403
[6]	曾晓雄. Kerr-Newman黑洞的熵修正. 物理学报, 2010, 59(1): 92-96. doi: 10.7498/aps.59.92
[7]	贺锋, 赵凡. 利用广义不确定关系计算Gibbons-Maeda黑洞的统计力学熵. 物理学报, 2009, 58(2): 740-743. doi: 10.7498/aps.58.740
[8]	崔大健, 林德华, 于海峰, 彭智慧, 朱晓波, 郑东宁, 景秀年, 吕力, 赵士平. 本征约瑟夫森结跳变电流分布的量子修正. 物理学报, 2008, 57(9): 5933-5936. doi: 10.7498/aps.57.5933
[9]	韩亦文, 洪云, 杨树政. 广义不确定关系与整体单极黑洞Dirac场的熵. 物理学报, 2007, 56(1): 10-14. doi: 10.7498/aps.56.10
[10]	周史薇, 刘文彪. 非对易时空下Gibbons-Maeda dilaton黑洞和Garfinkle-Horowitz-Strominger dilaton黑洞的热力学性质. 物理学报, 2007, 56(11): 6767-6771. doi: 10.7498/aps.56.6767
[11]	赵仁, 张丽春, 张胜利. 正则黑洞熵与相变. 物理学报, 2007, 56(12): 7355-7358. doi: 10.7498/aps.56.7355
[12]	赵仁, 张丽春, 张胜利. 正则黑洞熵. 物理学报, 2007, 56(7): 3719-3722. doi: 10.7498/aps.56.3719
[13]	刘晓莹, 张甲. 广义不确定关系与黑洞附近的热力学量. 物理学报, 2006, 55(11): 5638-5642. doi: 10.7498/aps.55.5638
[14]	刘成周, 赵峥. Gibbons-Maeda dilaton 黑洞的纠缠熵. 物理学报, 2006, 55(4): 1607-1615. doi: 10.7498/aps.55.1607
[15]	刘成周. 动态广义球对称含荷黑洞的量子熵. 物理学报, 2005, 54(5): 1977-1981. doi: 10.7498/aps.54.1977
[16]	王钢柱, 王纪龙. 缓变动态Kerr-Newman黑洞的量子热力学性质. 物理学报, 2004, 53(6): 1669-1674. doi: 10.7498/aps.53.1669
[17]	李固强. 自旋场对Barriola-vilenkin黑洞熵的量子修正. 物理学报, 2003, 52(6): 1346-1349. doi: 10.7498/aps.52.1346
[18]	林海. 满足热力学第三定律的修正的黑洞的熵公式. 物理学报, 2000, 49(8): 1413-1415. doi: 10.7498/aps.49.1413
[19]	李立新, 刘辽. 辐射在黑洞视界附近的性质与热力学第二定律. 物理学报, 1993, 42(1): 161-168. doi: 10.7498/aps.42.161
[20]	李富斌. 非平衡涨落问题的微观唯象分析理论(Ⅰ)——一种新的广义不可逆热力学理论与热涨落中涨落—耗散表示式的非平衡修正. 物理学报, 1989, 38(9): 1467-1474. doi: 10.7498/aps.38.1467

计量

文章访问数: 7910
PDF下载量: 81
被引次数: 0

姓名
邮箱
手机号码
标题
留言内容
验证码

搜索

留言板