[1]成天虎,朱轩然,任洳仪,等.De Sitter 时空下黑洞和宇宙视界面的热力学[J].西华师范大学学报(自然科学版),2017,38(01):101-105.[doi:10.16246/j.issn.1673-5072.2017.01.018]
 CHENG Tianhu,ZHU Xuanran,REN Ruyi,et al.The Thermodynamics of Black Hole and Cosmological Horizon in DeSitter Spacetime[J].Journal of China West Normal University(Natural Sciences),2017,38(01):101-105.[doi:10.16246/j.issn.1673-5072.2017.01.018]
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De Sitter 时空下黑洞和宇宙视界面的热力学()
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《西华师范大学学报(自然科学版)》[ISSN:1673-5072/CN:51-1699/N]

卷:
38
期数:
2017年01期
页码:
101-105
栏目:
出版日期:
2017-03-20

文章信息/Info

Title:
The Thermodynamics of Black Hole and Cosmological Horizon in DeSitter Spacetime
作者:
成天虎朱轩然任洳仪刘自祥
(西华师范大学 物理与空间科学学院,四川 南充637009)
Author(s):
CHENG TianhuZHU XuanranREN RuyiLIU Zixiang
(College of Physics and Space Science,China West Normal University,Nanchong Sichuan 637009,China)
关键词:
表面张力热力学第一定律视界
Keywords:
surface tensionsthe first law of thermodynamicshorizons
分类号:
P1456
DOI:
10.16246/j.issn.1673-5072.2017.01.018
文献标志码:
A
摘要:
首先分别计算了RessnerNordstrom de Sitter时空中黑洞视界面和宇宙学视界面的表面张力,并利用表面张力得到修改的热力学第一定律,它们满足相应的斯马尔关系式。在黑洞视界和宇宙视界,热力学第一定律呈现出不同的形式。
Abstract:
Firstly,the surface tensions of the black hole horizon plane and the cosmological horizon plane in ReissnerNordstrom de Sitter spacetime are calculated respectively.Then,the surface tensions are used to deduce the modified first law of thermodynamics that obey the corresponding Smarr relations.It is found that the law of the black hole horizon and the cosmology horizon take on different forms.

参考文献/References:


[1]HAWKING S W,PAGE D N.Thermodynamics of black holes in antide Sitter space[J].Commun.Math.Phys.,1983,87(4):577-588.
[2]CVETIC M,GUBSER S S.Phases of R charged black holes,spinning branes and strongly coupled gauge theories[J].JHEP,1999,1999(4):437-483.
[3]CVETIC M,GUBSER S S.Thermodynamic stability and phases of general spinning branes[J].JHEP,1999,1999(7):2193-2200.
[4]DOLAN B P.The cosmological constant and the black hole equation of state[J].Class.Quant.Grav.,2012,28(12):97-108.
[5]KUBIZNAK D,MANN R B.PV criticality of charged AdS black holes[J].JHEP,2012,2012(7):1-25.
[6]SEKIWA Y.Thermodynamics of de Sitter black holes:Thermal cosmological constant[J].Phys.Rev.D,2006,73(8):147-148.
[7]KASTOR D,RAY S,TRASCHEN J.Enthalpy and the mechanics of AdS black holes[J].Class.Quant.Grav.,2009,26(19):2551-2563.
[8]MIRZA B,SHERKATGHANAD Z.Phase transitions of hairy black holes in massive gravity and thermodynamic behavior of charged AdS black holes in an extended phase space[J].Phys.Rev.D.,2014,90,084006.
[9]JOHNSON C V.Holographic heat engines[J].Class.Quant.Grav.,2014,31(20):205002-205014.
[10]WANG S,WU S Q,XIE F.The first laws of thermodynamics of the (2+1)dimensional BTZ black holes and Kerrde Sitter spacetimes[J].Chin.Phys.Lett.,2006,23(2006):1096-1098.
[11]DOLAN B P,KASTOR D,KUBIZNAK D,et al.Thermodynamic volumes and isoperimetric inequalities for de Sitter black holes[J].Phys.Rev.D,2013,87(10):530-581.
[12]ZHAO H H,ZHANG L C,MA M S,et al.PV criticality of higher dimensional charged topological dilaton de Sitter black holes[J].Phys.Rev.D,2014,90(6):161-173.
[13]CAI R G.Connections between gravitational dynamics and thermodynamics[J].J.Phys.Conf.Ser.,2014,484(1):65-75.
[14]HANSEN D,KUBIZNAK D,MANN R B.Criticality and surface tension in rotating horizon thermodynamics[J].Class.Quant.Grav.,2016,33,165005.
[15]PADMANABBAN T.Classical and quantum thermodynamics of horizons in spherically symmetric spacetimes[J].Class.Quant.Grav.,2012,19(21):5387-5408.
[16]KOTHAWALA D,SARKAR S,PADMANABBAN T.Einstein’s equations as a thermodynamic identity:The cases of stationary axisymmetric horizons and evolving spherically symmetric horizons[J].Phys.Lett. B,2006,652(5/6):338-342.
[17]PADMANABHAN T,KOTHAWALA D.LanczosLovelock models of gravity[J].Phys.Rept.,2013,531(3):115-171.
[18]MISNER C W,SHARP D H.Relativistic equations for adiabatic,spherically symmetric gravitational collapse[J].Phys.Rev.B,1964,136(136):571-576.
[19]CAHILL M,MCVITTIE G.Spherical symmetry and massenergy in general relativity[J].I.general theory,J.Math.Phys.,1970,11(4):1392-1401.
[20]HU Y P,ZHANG H S.MisnerSharp Mass and the unified first law in massive gravity[J].Phys.Rev.D,2015,92,024006.
[21]HAYWARD S A.Quasilocal gravitational energy[J].Phys.Rev.D,1994,49(2):831-839.

备注/Memo

备注/Memo:

收稿日期:2016-08-18基金项目:国家自然科学基金项目(11205125);四川省青年基金(2014JQ0040);西华师范大学创新基金(438061)
作者简介:成天虎(1990—),男,重庆忠县人,硕士研究生,主要从事理论物理研究。
通信作者:刘自祥(1980—),男,四川雅安人,讲师,主要从事理论物理研究。E-mail: daivedlau@126.com
引用本文:成天虎,朱轩然,任洳仪,等.De Sitter时空下黑洞和宇宙视界面的热力学[J、.西华师范大学学报(自然科学版),2017,38(1):101-105.[CHENG Tianhu,ZHU Xuanran,REN Ruyi,et al.The thermodynamics of black hole and cosmological horizon in DeSitter spacetime[J].Journal of China West Normal University(Natural Sciences),2017,38(1):101-105.]De Sitter 时空下黑洞和宇宙视界面的热力学
更新日期/Last Update: 2017-03-20