Effect of Phantom Dark Energy on Holographic Thermalization
Xiao-Xiong Zeng1,2 , Xin-Yun Hu3** , Li-Fang Li4
1 School of Material Science and Engineering, Chongqing Jiaotong University, Chongqing 4000742 Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 1001903 School of Economics and Management, Chongqing Jiaotong University, Chongqing 4000744 State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190
Abstract ：Holographic thermalization for a black hole surrounded by phantom dark energy is probed. The result shows that the smaller the phantom dark energy parameter is, the easier the is plasma to thermalize as the chemical potential is fixed, the larger the chemical potential is, and the harder the plasma is to thermalize as the dark energy parameter is fixed. The thermalization velocity and thermalization acceleration are presented by fitting the thermalization curves.
收稿日期: 2016-10-20
出版日期: 2016-12-29
:
04.70.-s
(Physics of black holes)
04.70.Dy
(Quantum aspects of black holes, evaporation, thermodynamics)
04.25.dc
(Numerical studies of critical behavior, singularities, and cosmic censorship)
[1] Maldacena J M 1998 Adv. Theor. Math. Phys. 2 231 [2] Sonner J and Green A G 2012 Phys. Rev. Lett. 109 091601 [3] Li W J, Tian Y and Zhang H 2013 J. High Energy Phys. 1307 030 [4] Murata K, Kinoshita S and Tanahashi N 2010 J. High Energy Phys. 1007 050 [5] Ling Y, Niu C, Wu J, Xian Z and Zhang H 2014 Phys. Rev. Lett. 113 091602 [6] Hartnoll S A, Herzog C P and Horowitz G T 2008 Phys. Rev. Lett. 101 031601 [7] Cai R G and Yang R Q 2014 Phys. Rev. D 90 081901 [8] Mas J 2006 J. High Energy Phys. 0603 016 [9] Garfinkle D and Pando Z L A 2011 Phys. Rev. D 84 066006 [10] Garfinkle D, Pando Z L A and Reichmann D 2012 J. High Energy Phys. 1202 119 [11] Allais A and Tonni E 2012 J. High Energy Phys. 1201 102 [12] Das S R 2012 J. Phys.: Conf. Ser. 343 012027 [13] Steineder D, Stricker S A and Vuorinen A 2013 J. High Energy Phys. 1307 014 [14] Wu B 2012 J. High Energy Phys. 1210 133 [15] Gao X, Garcia-Garcia A M, Zeng H B and Zhang H Q 2014 J. High Energy Phys. 1406 019 [16] Buchel A, Lehner L, Myers R C and van Niekerk A 2013 J. High Energy Phys. 1305 067 [17] Keranen V, Keski-Vakkuri E and Thorlacius L 2012 Phys. Rev. D 85 026005 [18] Balasubramanian V et al 2011 Phys. Rev. Lett. 106 191601 [19] Balasubramanian V et al 2011 Phys. Rev. D 84 026010 [20] Baier R, Mueller A H, Schiff D and Son D 2001 Phys. Lett. B 502 51 [21] Galante D and Schvellinger M 2012 J. High Energy Phys. 1207 096 [22] Caceres E and Kundu A 2012 J. High Energy Phys. 1209 055 [23] Caceres E, Kundu A and Yang D L 2014 J. High Energy Phys. 1403 073 [24] Zeng X X and Liu W 2013 Phys. Lett. B 726 481 [25] Zeng X X, Liu X M and Liu W 2014 J. High Energy Phys. 1403 031 [26] Baron W H and Schvellinger M 2013 J. High Energy Phys. 1308 035 [27] Li Y Z, Wu S F and Yang G H 2013 Phys. Rev. D 88 086006 [28] Baron W 2013 J. High Energy Phys. 1303 070 [29] Arefeva I, Bagrov A and Koshelev A S 2013 J. High Energy Phys. 1307 170 [30] Hubeny V E, Rangamani M and Tonni E 2013 J. High Energy Phys. 1305 136 [31] Arefeva I Y and Volovich I V 2012 arXiv:1211.6041 [32] Belhaj A, Chabab M, El Moumni H and Sedra M B 2012 Chin. Phys. Lett. 29 100401 [33] Chen S B, Liu X F and Liu C Q 2013 Chin. Phys. Lett. 30 060401 [34] Balasubramanian V et al 2013 Phys. Rev. Lett. 111 231602 [35] Fonda P et al 2014 J. High Energy Phys. 1408 051 [36] Hubeny V E and Maxfield H 2014 J. High Energy Phys. 1403 097 [37] Zeng X X, Liu X M and Liu W 2015 Phys. Lett. B 744 48 [38] Giordano A, Grandi N E and Silva G A 2015 J. High Energy Phys. 1505 016 [39] Zhang S J, Wang B, Abdalla E and Papantonopoulos E 2015 Phys. Rev. D 91 106010 [40] Camilo G, Cuadros-Melgar B and Abdalla E 2015 J. High Energy Phys. 1502 103 [41] Buchel A, Myers R C and van Niekerk A 2015 J. High Energy Phys. 1507 137 [42] Zeng X X, Chen D Y and Li L F 2015 Phys. Rev. D 91 046005 [43] E Komatsu et al 2011 Astrophys. J. Suppl. Ser. 192 18 [44] Carroll S M, Hoffman M and Trodden M 2003 Phys. Rev. D 68 023509 [45] Hannestad S 2006 Int. J. Mod. Phys. A 21 1938 [46] Dunkley J et al 2009 Astrophys. J. Suppl. Ser. 180 306 [47] Gibbons G W and Rasheed D A 1996 Nucl. Phys. B 476 515 [48] Azreg-Aïnou M, Clément G, Fabris J C and Rodrigues M E 2011 Phys. Rev. D 83 124001 [49] Rodrigues M E and Oporto Z A A 2012 Phys. Rev. D 85 104022 [50] Azreg-Aïnou M 2013 Phys. Rev. D 87 024012 [51] Gyulchev G N and Zh S I 2013 Phys. Rev. D 87 063005 [52] Maldacena J M 1998 Phys. Rev. Lett. 80 4859 [53] Ling Y, Niu C, Wu J P and Xian Z Y 2013 J. High Energy Phys. 1311 006
[1]
.
[2]
.
[3]
.
[4]
.
[5]
.
[6]
.
[7]
.
[8]
.
[9]
.
[10]
.
[11]
.
[12]
.
[13]
.
[14]
.
[15]
.
2017, Vol. 34 
