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JHEP03(2018)056
Published for SISSA by Springer
Received: October 26, 2017
Accepted: February 13, 2018
Published: March 9, 2018
Diffusion for holographic lattices
Aristomenis Donos ,
a
Jerome P. Gauntlett
b
and Vaios Ziogas
a
a
Centre for Particle Theory and Department of Mathematical Sciences, Durham University,
Durham, DH1 3LE, U.K.
b
Blackett Laboratory, Imperial College,
London, SW7 2AZ, U.K.
E-mail:
aristomenis.donos@durham.ac.uk, j.gauntlett@imperial.ac.uk,
vaios.ziogas@durham.ac.uk
Abstract: We consider black hole spacetimes that are holographically dual to strongly
coupled field theories in which spatial translations are broken explic i tly. We discuss how
the quasinormal modes associated with diffusion of he at and charge can be systemati c al l y
constructed in a lon g wavelength pertur bat i ve expansion. We show that the dispersion
relation for these modes is given in t er ms of the thermoelectr i c DC conductivity and static
susceptibilities of the dual field the or y and thus we derive a generalised Ei ns te i n relation
from Einstein’s equations. A corollary of our results is t hat thermodynamic instabilities
imply specific type s of dynamical instabilities of the associated black hole solutions.
Keywords: AdS-CFT Correspondence, Bl ack Holes in String Theory, Holography and
condensed matter physics (AdS/CMT)
ArXiv ePrint: 1710.04221
Open Access,
c
The Authors.
Article funded by SCOAP
3
.
https://doi.org/10.1007/JHEP03(2018)056
JHEP03(2018)056
Contents
1 Introduction
1
2 Background black hole solutions 4
2.1 Susceptibilities from the horizon 5
3 Time dependent perturbation and the constraints 6
3.1 Constraints 7
4 Constructing the bulk diffusion perturbations 8
4.1 Dispersion relations for the diffusion modes 10
4.2 Comments 13
5 Final comments 16
A Residual gauge invariance 17
B Evaluating the cons tr aints on the horizon 17
B.1 Constraints in the radial decomposition 17
B.2 Evaluating constraints for the perturbation 18
C Calculating the DC conductivity 21
D Counting functions of integration 22
E Fixing the zero modes of the ε expansion 24
1 Introduction
Holography provides a powerful theoretical framework for studying the propert i e s of
strongly coupled quantum criti cal syst em s. A basic feature is that a given quantum sys-
tem in thermal equilibrium is described by a stationary black hole spacetime with a Killing
horizon and, furthermore, the entropy and conserved charges can be universally determined
by data on the black hole horizon (e . g. see [
1] and references therein). Going beyond ther-
mal equilibrium and moving to the realm of linear response, it has been shown that the
thermoelectric DC conductivity, when finite, is also universall y determined by data on the
horizon, by solvin g a specific Stokes flow for an auxiliary fluid on the horizon [
2] (further
extensions are di sc us se d in [
3–6]).
It is natural to enquire if other prope rt i e s of the dual field theory can also be obtained
from horizon d ata. In thi s paper we discuss the construction of quasi-nor mal modes that
– 1 –
JHEP03(2018)056
are dual to the long wave-length hydrodynamic modes associated with diffusion of heat
and electric charge. In particular, we will show how the dispersi on relation for these modes
can also be obtained in terms of the properties of the black hole solutions at the horiz on.
Recall that in the specific context of translationally invariant and charge neutral sys-
tems the diffusion of electric charge was first discusse d some time ago in [7]. Furthermore,
again for thi s specific setup, an Einstein relation, relating the associate d elect r i c diffusion
constant to the finite DC conducti v i ty and stat i c charge suscepti bi l i t i es , was derived in [
8],
where it was also shown how the DC conductivity can be obtained explici t l y from the
horizon.
1
It should be noted that in this set up the thermal DC conductivity is infinite
and, corr e spondingly, there is no heat diffusion mode . In this paper we wi l l discuss the dif-
fusion of both electric charge and heat within the general context of charged and spatially
inhomogeneous media. The spati al inhomogeneities that we consider arise from breaking
of spatial translations explicitly, and the black holes are known as ‘hologr aphi c lattices’ [9].
In a recent paper [
10] we carried out an analysis of the diffusion of conserved charges
in the context of spatially inhomogeneous media for arbitrary quantum field theories (not
necessarily hol ogr aphi c ) . Subject to the retarded current-current cor r el at or s satisfying
some general analyticity conditions, as well as assuming that the thermoelectric DC con-
ductivity is finite, the long wavelength hydrodynamical modes associate d with diffusion of
charge and heat were identified and a generalised Einstein rel at i on was derived. In addi-
tion, the general formalism was il l ust r ate d for thermoelectric diffusion within the context
of relativis ti c hydrodynamics where momentum dissipation was achieved not by modifying
the conservati on equations, as is usually done, but by explicitly breaking translations by
considering the system with spati al l y modulated sources for the stress tensor and electric
current as in [
11, 12].
Given the general results presented in [
10], one anticipates that it shoul d be possible to
derive the generalised E i nst e i n relations within the context of general classes of holographic
lattices. Specifically, we will consider cases in which the DC conductivity is finite
2
and e q ual
to a horizon DC conductivity that is obtained by solving a Stokes flow on the horizon. One
can then ask about the relevant charge susceptibilities. Since the conserved charges can
be evaluated at the horizon provided one knows how this data depends on changing the
temperature and the chemical potential of the black holes in thermal eq u i l i br i um, one
can also obtai n horizon expressions for the susceptibilities. As we wil l see, this simple
observation about the susceptibilities will be sufficient to extract the dispersion relations for
the diffusive mode s and hence the Ei ns te i n re l ati on. In slightly more detail, using a radial
decomposition of the eq uat i ons of motion, we will explain how the quasi -nor mal diffusion
modes can be systematically constructed in a long wavelength, perturbative expansion. In
general, while both the radial equations and the constraint equations are required to carry
out this construction, we will see that an analysis of just the constraint equations on the
horizon are sufficient to extract the Ei nst e i n relation, which is the universal part of the
dispersion relation in the long wavelength expansion for the diffusive modes.
1
From the universal perspective of [
2], this is a special set up where the Stokes flow equations are solved
trivially.
2
In particular, we will not be considering superflu id s .
– 2 –
JHEP03(2018)056
Recently there has been a particular focus on studying diffusion of heat and charge in
the context of holography. This stems, in part, f r om the suggestion that diffusive processes
may be a key to understanding universal aspects of transport in incoherent metals [
13].
Furt her m ore , it was also suggested in [
13] that there m i ght be lower bounds on diffusion
constants by analogy with bounds on shear viscosity associated wi t h diffusion of momen-
tum [
14]. A key idea is to write D ∼ v
2
τ, where D is suitabl e diffusi on constant and v, τ
are characteristic velocities and time scales of the system, and it was suggested in [
13] that
τ should be the ‘Planckian time scale’ τ = ~/(k
B
T ) [
15, 16]. An interesti ng subsequent
development was the suggestion that v should be identified with the butterfly velocity, v
B
,
extracted from out of time order cor r e l ator s [
17, 18] and used as a measure of the onset of
quantum chaos.
While there has been a r ange of interesti ng holographic results in this dir ec ti on , includ-
ing [
19–32], wit h an appreciation that it is the thermal diffusion should be rel at e d to v
B
, it
is fair to say that within hol ograp hy a sharp global picture has yet to emerge.
3
Almost all
of the holographic stud y in this area has b e e n in the setting of sp e c i fic types of ‘homoge-
neous’ hologr aphi c lattices [
41, 42], which maintain a translationally invariant metric. In
these cases it is straightforward to extract v
B
by studying a sh ock wave entering the black
hole horizon [
43, 44] (see also [45]). A notabl e exception is [19] who studied holograp hi c
lattices in one spatial dimension, but working in a hydrodynamic, high temperat ur e li mi t
of the background hol ogr aphi c lattice. We hope that the present work, which illuminates
universal aspects of diffusion for arbitrary spatial modulation in holography, will be useful
in further developments.
In a di ff er e nt direction, our derivation of the dispersion relation lead s to a general
connection between thermodynamic instabilities and dynamic instabilities. Some tim e ago,
building on [
46, 47], it was shown in a spe cific holographic context with a translationally
invariant horizon, that thermodynamic instability implies an imaginary speed of sound,
leading to unstable quasi-normal modes and dynamical instability
4
[52]. For general spatial
modulation within holography, any sound modes will onl y appear on scal e s much smaller
than the scale of the modulation and he nc e this wi l l not be a universal channel to deduce
dynamical instability from thermodynamic instability. Instead, the diffusion modes do
provide such a channel. Specifically, in the presence of spatial modulation, we can deduce
the following result. If the heat and charge susceptibility matrix has a negative e i genvalue,
then the system is thermody n ami cal l y unstable and then the dispersion relati on implies
that t he re is at least one mixed diffusion mode, involving heat and charge, living in the
upper half plane which will necessarily lead to a dynamic al instability.
3
It is striking that a relation of the f or m D ∼ v
2
B
τ has also appeared in a variety of other non-holographic
contexts, including [
22, 33–40], with τ ∼ λ
−1
L
where λ
L
is the Lyapunov exponent [35].
4
Some recent discussion of both hydrodynamic and n o n -hydrodynamic modes and the connect io n with
instabilities in a translationally invariant setting, appeared in [
48–51].
– 3 –
JHEP03(2018)056
2 Background black hole solutions
We will consider a general class of bulk theories which couple the metric to a gauge field
A
µ
, with field strength F
µν
, and a scalar field φ in D spacetime dimensions, governed by
an action of the form
S =
Z
d
D
x
√
−g
R − V (φ) −
Z(φ)
4
F
2
−
1
2
(∂φ)
2
. (2.1)
The only constraints that we impose on the functions V (φ), Z(φ) is that the equations of
motion admit an AdS
D
vacuum soluti on with φ = A
µ
= 0. We assume that in this vacuum
the scalar field φ is dual to an operator with conformal dimension ∆. We have also set
16πG = 1 for c onvenience.
We are interested in studying the family of static, background black hole solutions that
lie within the ansatz
ds
2
= − U G dt
2
+
F
U
dr
2
+ ds
2
(Σ
d
) ,
A = a
t
dt , (2.2)
with ds
2
(Σ
d
) = g
ij
dx
i
dx
j
and d = D − 2. The functions G, F, a
t
, φ and the metric compo-
nents g
ij
are all independent of the time coordinate t and depend on (r, x
i
). Note that the
function U = U(r), which is redundant, is included to conveniently deal with some aspects
of the asymptotic behaviour of the solution.
Although it is possible to be more general, to simplify the presentation we will assume
that we have single black hole Killing horizon, located at r = 0, and that the coor di n ate s
(t, r, x
i
) are globally defined outside t he black hole all the way out to the AdS
D
boundary
which will be located at r → ∞. In particular, this means that the radial foliation is
globally defined up to a ‘stretched horizon’ located at some small radial distance outside
the black hole and that the t opology of the black hole horizon is Σ
d
. Similarly, we will
also assume Σ
d
has planar topology and all functions appearing in (
2.2) are assumed to
be periodic in the spatial directions x
i
with period L
i
, correspond i ng to static, peri odic
deformations of the dual CFT. It will be useful to define
H
= (
Q
L
i
)
−1
R
dx
1
. . . dx
d
which
allows us to extract the zero mode of periodic functions .
Asymptotically, as r → ∞, the solutions are taken to approach AdS
D
with boundary
conditions that e x pl i c i t l y break translation invariance:
U → r
2
, F → 1, G → G
(∞)
(x), g
ij
(r, x) → r
2
g
(∞)
ij
(x),
a
t
(r, x) → µ( x) , φ(r, x) → r
∆−d−1
φ
(∞)
(x) . (2.3)
This cor r e sponds to placing the dual CFT on a curved spacetime manifol d with metric given
by ds
2
= −G
(∞)
(x)dt
2
+ g
(∞)
ij
(x)dx
i
dx
j
, having a spatially dependent chemical potential
µ(x) and d efor m i ng by a spatially dep e nde nt source φ
(∞)
(x) for t he operator dual to φ. It
will be c onvenient to separate out the zero mode of µ(x) by defining
µ(x) ≡ ¯µ + ˜µ(x) (2.4)
with constant ¯µ and
H
˜µ(x) = 0.
– 4 –
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