-
1
-
-
84952363681
-
-
general, the result (Equation presented) will not be valid for translationally invariant anisotropic black holes nor for holographic lattices
-
In general, the result (Equation presented) will not be valid for translationally invariant anisotropic black holes nor for holographic lattices.
-
-
-
-
12
-
-
61549123354
-
-
N. Iqbal and H. Liu, Phys. Rev. D 79, 025023 (2009). PRVDAQ 1550-7998 10.1103/PhysRevD.79.025023
-
(2009)
Phys. Rev. D
, vol.79
, pp. 025023
-
-
Iqbal, N.1
Liu, H.2
-
13
-
-
0000466068
-
-
R. Price and K. Thorne, Phys. Rev. D 33, 915 (1986). PRVDAQ 0556-2821 10.1103/PhysRevD.33.915
-
(1986)
Phys. Rev. D
, vol.33
, pp. 915
-
-
Price, R.1
Thorne, K.2
-
14
-
-
40549131295
-
-
S. Bhattacharyya, V. E. Hubeny, S. Minwalla, and M. Rangamani, J. High Energy Phys. 02 (2008) 045. JHEPFG 1029-8479 10.1088/1126-6708/2008/02/045
-
J. High Energy Phys.
, vol.2008
, Issue.2
, pp. 045
-
-
Bhattacharyya, S.1
Hubeny, V.E.2
Minwalla, S.3
Rangamani, M.4
-
16
-
-
58149481708
-
-
I. Fouxon and Y. Oz, Phys. Rev. Lett. 101, 261602 (2008). PRLTAO 0031-9007 10.1103/PhysRevLett.101.261602
-
(2008)
Phys. Rev. Lett.
, vol.101
, pp. 261602
-
-
Fouxon, I.1
Oz, Y.2
-
17
-
-
84864447901
-
-
I. Bredberg, C. Keeler, V. Lysov, and A. Strominger, J. High Energy Phys. 07 (2012) 146. JHEPFG 1029-8479 10.1007/JHEP07(2012)146
-
J. High Energy Phys.
, vol.2012
, Issue.7
, pp. 146
-
-
Bredberg, I.1
Keeler, C.2
Lysov, V.3
Strominger, A.4
-
18
-
-
35148892646
-
-
S. A. Hartnoll, P. K. Kovtun, M. Muller, and S. Sachdev, Phys. Rev. B 76, 144502 (2007). PRBMDO 1098-0121 10.1103/PhysRevB.76.144502
-
(2007)
Phys. Rev. B
, vol.76
, pp. 144502
-
-
Hartnoll, S.A.1
Kovtun, P.K.2
Muller, M.3
Sachdev, S.4
-
19
-
-
84941334800
-
-
M. Blake, J. High Energy Phys. 09 (2015) 010. JHEPFG 1029-8479 10.1007/JHEP09(2015)010
-
J. High Energy Phys.
, vol.2015
, Issue.9
, pp. 010
-
-
Blake, M.1
-
21
-
-
84952363683
-
-
For simplicity, we set (Equation presented) and also set the cosmological constant to a convenient value
-
For simplicity, we set (Equation presented) and also set the cosmological constant to a convenient value.
-
-
-
-
22
-
-
84952363684
-
-
The time-dependent piece in (16) implies the static susceptibility of the heat current two-point Green's function is proportional to (Equation presented); see [10,11]
-
The time-dependent piece in (16) implies the static susceptibility of the heat current two-point Green's function is proportional to (Equation presented); see [10,11].
-
-
-
-
23
-
-
84952363685
-
-
Some examples where the horizon transport quantities are, accidentally, the same as the in the field theory case are discussed in [2,3,12]
-
Some examples where the horizon transport quantities are, accidentally, the same as the in the field theory case are discussed in [2,3,12].
-
-
-
-
24
-
-
84952363686
-
-
Other topologies will be discussed in [20]
-
Other topologies will be discussed in [20].
-
-
-
-
25
-
-
84952363687
-
-
The one-dimensional case was studied in [27,28]
-
The one-dimensional case was studied in [27,28].
-
-
-
|