###### Abstract

We present the results of our studies of the entanglement entropy of a superconducting system described holographically as a fully back–reacted gravity system, with a stable ground state. We use the holographic prescription for the entanglement entropy. We uncover the behavior of the entropy across the superconducting phase transition, showing the reorganization of the degrees of freedom of the system. We exhibit the behaviour of the entanglement entropy from the superconducting transition all the way down to the ground state at . In some cases, we also observe a novel transition in the entanglement entropy at intermediate temperatures, resulting from the detection of an additional length scale.

0.5in

Holographic Studies

of

Entanglement Entropy in Superconductors

Tameem Albash, Clifford V. Johnson

Department of Physics and Astronomy

University of Southern California

Los Angeles, CA 90089-0484, U.S.A.

talbash, johnson1, [at] usc.edu

## 1 Introduction

Given a quantum system, the entanglement entropy of a subsystem and its complement is defined as follows:

(1) |

where is the reduced density matrix of given by tracing over the degrees of freedom of , , where is the density matrix of the system.

The entanglement entropy is understood as an important probe of physics in various domains, and for systems at strong coupling it is looked upon as a robust tool for keeping track of the degrees of freedom when other traditional probes (such as an order parameter) might not be available. However, it is often difficult to compute the entanglement entropy in such systems, especially outside 1+1 dimensions.

Two developments in the field have made the work in this paper possible. The first is that the entanglement entropy has a natural geometrical
definition [1, 2] (proposed but only partially proven^{1}^{1}1See e.g.,
refs. [3, 4, 5, 6, 7, 8, 9, 10]..) in the context of gauge/gravity duals, where a wide class of strongly coupled theories in dimensions can be defined holographically as dual to a theory of gravity (plus other degrees of freedom) in dimensions, which is in turn ultimately embedded into a 10 dimensional superstring theory or an 11 dimensional supergravity background as a means of ensuring full quantum consistency. Of course, holography is also not fully proven, but there is a large body of evidence for it in numerous examples, starting with the AdS/CFT correspondence and deformations and generalizations thereof [11, 12, 13, 14]. In this paper we shall assume that holography is robust, and that the holographic formula (reviewed below) for the entanglement entropy is also correct.

The second development is that some of the strongly coupled physics of interest, superconducting^{2}^{2}2To be precise, the physics breaks a global, not local, symmetry, but it is close to being gauged, in a sense [15]. So rather than using the term superfluidity, we will continue with the common usage. phases that share various features with certain exotic phases of experimentally studied strongly coupled quantum systems, can not only be modelled holographically as an effective model of gravity plus a scalar (see e.g. ref. [16]), not only be embedded consistently into the parent superstring theory and/or 11D supergravity to get access to the back reactions of the scalar dynamics on the geometry (see e.g. ref. [17]), but can be embedded in a manner that appears to be highly stable^{3}^{3}3Strictly speaking, the stability is typically studied in various truncations of 11D supergravity to lower dimensions. We mean here full perturbative stability of the ground state in maximal supergravity in 4D. There remains the possibility of instabilities arising upon uplift to the full 11D supergravity, non–perturbative instabilities, and parts of the phase diagram being modified at higher temperatures by instabilities of the sort discussed in e.g. ref.[18]. (i.e., refs. [19] and [20] have shown that the ground states of an infinite subset of the family of superconductors defined by the embeddings in ref. [17] are in fact unstable in maximal supergravity in 4D and it remains to be shown whether any of the others in the family are stable). In other words, there is a holographic superconductor model (presented recently in ref. [21]) that has a ground state that, thought of as a holographic flow[22]
is a stable^{4}^{4}4Subject to the caveats in the previous footnote. non–supersymmetric vacuum of the full theory. This suggests that the complete theory of gravity plus all the attendant fields is without pathological physics that might obscure the lessons to be learned from it about strongly coupled phenomena pertinent to the superconductivity.

These two developments come together nicely since to employ the holographic definition of the entanglement entropy in a study of superconductivity, we need the complete (back–reacted–upon and stable) geometry to perform the computation. In this paper we carry out the study of the entanglement entropy in holographic superconductivity for the first time using these methods, and uncover some very interesting phenomena.

The entropy is holographically computed as follows [1, 2]. In an asymptotically Anti–de Sitter (AdS) geometry, consider a slice at constant AdS radial coordinate . Recall that this defines the dual field theory (with one dimension fewer) as essentially residing on that slice in the presence of a UV cutoff set by the position of the slice. Sending the slice to the AdS boundary at infinity removes the cutoff (see ref. [23] for a review). On our slice, consider a region . Now find the minimal–area surface bounded by the perimeter of and that extends into the bulk of the geometry. (Figure 1 shows examples of the arrangement we will consider in this paper.) Then the entanglement entropy of region with is given by:

(2) |

where is Newton’s constant in the dual gravity theory.

In the next section, we will review the four dimensional model of gravity plus scalars and a gauge field that was presented in ref. [21], and review and re–derive the properties of the solutions we need.

## 2 Gravity Background

The Lagrangian of ref. [21] arises as an invariant truncation of four–dimensional gauged supergravity:

(3) |

where the potential is given by:

(4) |

We use a different notation from ref. [21]. We first reintroduced the dimensionful constant and then made the following field redefinitions:

(5) |

Note that the gauge field and the (real) scalar fields and are dimensionless in this framework.

The metric and other fields of interest are parameterized as follows:

(6) |

and the scalar will be set to zero. Defining a useful dimensionless coordinate:

(7) |

the equations of motion can be reduced to:

(8) | |||

(9) | |||

(10) | |||

(11) |

The ultraviolet (UV) asymptotic behavior (near the AdS boundary ):

(12) |

Generically we will be at finite temperature, to which there will be associated an event horizon in the geometry. We assume the event horizon occurs at , and near there the fields have an expansion:

(13) |

There are only three independent parameters here, which we choose to be . There are three scaling symmetries of the equations of motion given by [21]:

(14) | |||

(15) | |||

(16) |

Using these scaling symmetries, we can choose any value for the position of the event horizon and the asymptotic value of the field . We choose to fix and , and tune to either have or be zero. These asymptotic values of the field in the UV define the vacuum expectation value (vev) of charged operators in the theory that are either of dimension 1 or 2, and we correspondingly call them and . We will explicitly identify the correctly normalized relationship below. The UV asymptotics of the electric gauge field component defines a chemical potential and charge density that will be explicitly identified below.

Generically, a solution will have non–zero. To recover pure AdS, we use the scaling symmetry in equation (14) to shift as:

(17) |

which can be accomplished by rescaling the time coordinate:

(18) |

which in turn means:

(19) |

The temperature of the system is then given by [21]:

(20) |

and the chemical potential and charge density go as:

(21) |

and the vevs of the two operators are defined as:

(22) |

Using the scaling symmetry in equation (16), the relevant quantities for us scale as:

(23) |

Therefore, we will use the following dimensionless quantities to examine the physics:

(24) |

### 2.1 High Temperature Phase

At high temperature, the solution is simply the Reissner–Nordström AdS solution. The scalar profile being zero means that there is no condensate, i.e., the operators and vanish. The solution is given by taking (we restore dimensionful for now):

(25) |

So we read off the temperature, chemical potential, and density as:

(26) |

### 2.2 Intermediate Temperature Phase

At low enough temperatures, a new type of solution is available that is a charged black hole with a non–zero charged scalar profile. We have non–zero and , and we require either or , corresponding to having either or turned on respectively.

The solutions can only be exhibited numerically, and we display the resulting plots of temperature versus operator vev for each case of and in figure 2. Below a critical temperature , this type of solution is thermodynamically favored over the Reissner–Nordström case, and represents the superconducting phase, with non–zero condensate. These thermodynamics will be reviewed in the next section.

### 2.3 Zero Temperature Phase

The zero temperature solution is an RG flow between two AdS spaces[21]. In the IR, the fields have the behaviour:

(27) |

where

(28) |

### 2.4 Thermodynamics

The on–shell regularized action is given by:

(29) |

where we have used the equations of motion to simplify the on–shell action. The quantity is the volume of the upon which the field theory resides. Putting everything in we get [21]:

(30) |

where is the Gibbs energy density. So we define the free energy density as:

(31) |

The Reissner–Nordström free energy density is given by:

(32) |

where are found by solving:

(33) |

We define the difference of the free energy densities:

(34) |

We show the free energy density difference as function of temperature in figure 3, for each case of and . When , there is a transition from Reissner–Nordström to the black hole with scalar profile, representing the superconducting phase. This defines the phase transition temperature, .

Note that in the case of , it is the upper branch (the choice with higher vev for ) that is favoured. Here, in contrast to the case where the vev rises continuously from zero at , the operator has a jump in the vev at . The physics of these cases is described more in ref.[21].

It is worth noting here that while the phase structure in the case seems strikingly different from that of , we are aware of another model in the literature that shows how the two can be connected, although using an apparently different mechanism. In refs. [24, 25], the introduction of a background current in the can continuously deform the solution space of the into that of the case. Here, instead of a current, the unusual behaviour of the metric function is responsible for the multivaluedness of available scalar black holes for some ranges of temperatures. In either way of thinking about it, there is a new length scale in the theory that manifests itself as a finite value in the jump of the free energy and of as the transition temperature is crossed. As we will see, the entanglement entropy will be able to detect this new length scale.

## 3 Entanglement Entropy

With a complete supergravity solution in hand, we are ready to study the entanglement entropy at each temperature and study the physics.. We use a strip geometry, as outlined in the introduction. We choose the following embedding:

(35) |

The resulting entanglement entropy is given by:

(36) |

The extremization problem has a constant of the motion given by:

(37) |

where is the location in of the bottom of the extremal surface. This allows us to write the entanglement entropy as:

(38) |

where has dimensions of inverse length with no divergences. The length is given in terms of :

(39) |

Under this scaling of equation (16), and scale as:

(40) |

so we will focus on the following dimensionless quantities:

(41) |

We are now ready to explore the results.

### 3.1 Superconductor

We show in figure 4 the results for obtained by fixing the temperature and varying , the width of the strip. Larger probes more deeply into the infra–red. We show cases with temperature below the transition temperature . (At the transition temperature, the curves for the Reissner–Nortström case and the scalar charged black hole (representing the superconducting phase) are identical.) In all cases, the curves go linearly with for large as is expected from the area law. As the temperature is lowered, the slope of the curve for large (still linear) is smaller for the superconducting background, and continues to flatten out as we approach zero temperature. This is expected since for , the background is an RG flow from one AdS vacuum to another, and this flattening out of the entanglement entropy at some finite value was observed in our studies of entanglement entropy along RG flow presented in ref. [26].

The fact that for a particular , the superconducting solution exhibits a lower entropy than the Reissner–Nordström solution fits with the expectation that degrees of freedom have condensed and so there should be fewer of them.

It is instructive to slice the data differently, fixing a strip width and studying how the entropy of the system changes with temperature. We present this in figure 5. In reading the figure, determine the physical curve by always choosing the point of lowest entropy at a given . A discontinuity in the slope of the decreasing entanglement entropy can be observed at the transition temperature (indicated by the vertical dotted line), showing its utility as an independent probe of the phase structure of the superconductor.

The slope may be thought of as a sort of response function characterizing the system, roughly analogous to a specific heat. It is natural for it to be positive, since increasing temperature should indeed promote entanglement entropy. A discontinuous change in the slope at the transition temperature signifies a significant reorganization of the degrees of freedom of the system. Since there is a condensate generated, it is also to be expected that there is a reduction in the number of degrees of freedom as well, although precisely at , the condensate value only just begins to rise from zero. We will see something more dramatic in the case, by way of contrast.

### 3.2 Superconductor

We show in figure 6 the results for obtained by fixing the temperature and varying , the width of the strip. As before, larger probes more deeply into the infra–red. We again show cases with temperature below the transition temperature , although in this case, at , the Reissner–Nordström curve lies above that of the superconductor curve. This will mean a discontinuous jump in the value of the entropy, as we will see below, in contrast to the case. For all cases, the typical behavior of the curve initially resembles that of the case, in that the curve of the superconducting solution has a lower slope. However, for , we find multiple solutions for a given range of strip widths , which form a swallowtail shape in our curves. This means there is a kink in the physical curve for the entanglement entropy, since we must choose the lowest value. For future reference, we will refer to the two parts of such kinked curves as the “small ” branch and the “large ” branch, respectively, going from small to large .

The kink moves to lower strip widths as the temperature is decreased (for fixed charge density), and persists at zero temperature. Another interesting point is that the leveling off of the curve at zero temperature occurs at a positive finite value. This is interesting since in ref. [26], only negative finite values were observed. Furthermore, the case of the previous subsection also exhibits a negative finite value. In ref. [26], we predicted from our sharp domain wall analysis that a positive finite value would develop if the domain wall was sufficiently sharp and near the UV. We will explore this in subsection 3.4.

It is also interesting to track, as a function of temperature, the strip width value, , at which the kink appears in the entanglement entropy. We do this in figure 7. (Note also that, for fixed temperature, .) From this curve we can read off an interesting piece of information. If we pick a specific strip width value between an and an we can read off a specific temperature at which the entanglement entropy is crossing over from the “small ” branch of an curve to the “large ” branch of the curve, the branches being separated by a kink. The significance of this temperature will be apparent shortly.

A swallowtail multivaluedness in the entanglement entropy, showing multiple extremal surface solutions at a given , was first observed and characterized in our studies, presented in ref. [27], of the evolution of the entanglement entropy after a quenching process^{5}^{5}5Refs.[28, 29] have also since observed this phenomenon.. We will discuss the origins of the multivaluedness of the present case in the next subsection.

Physically, the appearance of a kink in the entanglement entropy as we go to larger can be attributed to sensitivity to a new scale in the theory, and the entanglement entropy is a good probe of its presence. In contrast to the case, the transition at was associated with a finite jump in the free energy , and also a jump in the the vev of the operator . This sets and additional scale in the theory that distinguishes it from the case. (See also our discussion, near the end of section 2.4, of this scale and how it can arise from the addition of a background current in the probe limit.) The basic scale, which we can denote , is set by the inverse of the discontinuity of the vev of at . For subsequent temperature an effective scale follows from this, by RG flow. For very small strip size , the entanglement entropy will not be sensitive to , but when becomes comparable to , our results suggest that correlations between quanta on these scales effectively reduce the number of effective degrees of freedom, reducing the contributions to the entanglement entropy, resulting in a kink to change of the slope of the curve for larger . The details of how this works from the field theory perspective, and the kink’s fate away from the large limit, would be interesting to explore further, in future work.

As was done for the case of , it is instructive to study the entropy for fixed as the temperature varies. There are in fact three distinct situations, giving rise to three different types of curve. The distinguishing issue is whether the choice of fixed can ever become a kink value, , at some temperature. As we saw, figure 7 has the answer to this.

The first case is to have a fixed that is greater than . Then, at successively lower temperatures than , the entropy will always come from points on “large ” branches of curves, since the kink moves to smaller as is reduced. We show the resulting type of curve in figure 8. In this and the next two figures, the red curve is always favoured for , indicated by the vertical dotted line. Below , one should determine the physical curve by always choosing the point of lowest entropy at a given . Notice how the region of negative slope is nicely avoided. This will be the case in our subsequent curves as well.

The second case is to have a fixed that is smaller than . There is no temperature at which this would become a kink value, since although the kink moves to smaller with smaller , it stops at at . So the contributions to the entropy come entirely from points on “small ” branches of curves. We show the resulting type of curve in figure 9.

The final case is to have a fixed such that . Then, as we reduce the temperature from , entropy contributions are from “large ” branches until a temperature is reached such that our chosen is a kink value . This temperature can be read off from figure 7. For lower temperatures, the entropy will be from points on “small ” branches. Consequently, the superconductor phase of the curve in this case will be a combination of two types of curve, connected by a new discontinuity in the derivative where they join. We show the resulting type of curve in figure 10.

In all the curves in figures 8, 9 and figure 10, we see that in addition to the slope having a discontinuity at the transition temperature (shown by the vertical dotted line), the value of the entropy drops discontinuously as well, as we earlier anticipated. Then, when , we have the additional feature of a discontinuity in the slope at some lower temperature, generated (as discussed above) by the sensitivity to the length scale . Note that for fixed with a value close to the edges (but outside) of this interval, the resulting curves will appear to have a locally smoothed out discontinuity. The cases displayed here are far away enough from the interval that the smoothing is spread out.

### 3.3 Multivaluedness of the Entanglement Entropy

As stated already, we’ve seen a multivaluedness of the entanglement entropy before, in a study of its evolution after a quench [27]. This resulted in a kink representing the change in the saturation rate of the entropy as it evolved. To understand the reason for the appearance of the multivaluedness in this case, we study the behavior of the function , which we show examples of in figure 12 (we show the behavior for the function in figure 11 for comparison purposes). Slightly before the rightmost point in the vev curve of figure 2(b), develops two new extrema, a minimum and a maximum. The maximum grows higher in value and the minimum becomes sharper (i.e. greater second derivative) as the temperature decreases. Both extrema move toward the AdS boundary at (the UV) as the temperature decreases.

We show the behavior of the function at zero temperature in figure 12(b). As for the finite (but low) temperature case, the function has a minimum. This minimum is now a finite distance from the UV boundary, and the maximum we saw at finite temperature has now smoothed out to a constant as we go toward the IR.

It is the non–monotonic behavior of that generates the multivaluedness, as illustrated in figure 13. When , the location of the lowest point of the extremal surface, is in the neighborhood of the minimum of , the entanglement entropy becomes multivalued. Only when relatively far from the minimum does the entanglement entropy become single–valued again.

### 3.4 Domain Wall Behaviour

The non–monotonic behavior of suggests that the behavior of the domain wall that interpolates between the two AdS vacua (at zero temperature) is also not monotonic. In addition, we’d also like to compare the domain wall features of the cases and , to see if we can understand the differences between the large saturation values of the entanglement entropy observed in sections 3.1 and 3.2 (negative versus positive) in the terms discussed in our RG flow studies of ref. [26]. To study this, we first write the metric in the following form:

(42) |

The function encodes the domain wall, and the coordinate can be determined via:

(43) |

Note that technically is actually at since that corresponds to the IR of the theory. So to circumvent this issue, we can define a variable such that:

(44) |

and simply shift our result for by a constant such that the ratio does not diverge at . We show the behavior of in figure 14. Indeed, as expected, it is non–monotonic for the case, and indeed the domain wall is much sharper for this case than it is for the case, confirming our observations made in section 3.2 and ref. [26] about the saturation of the entanglement entropy at large at . The multivaluedness feeds nicely into the swallowtail structure, as we saw in the previous section by looking directly at .

## 4 Concluding Remarks

Since we have carefully unpacked and discussed our results during our presentation of them, we will be brief in this section.

We have presented a study, using holography, of the entanglement entropy of a certain type of strongly coupled superconductor. Since the background is fully backÐreacted and highly stable (in the sense outlined in footnote 3), we can be confident that the results are robust.

This is the first such study of its type, and the results may well be of interest beyond the confines of holography, since it is of interest in the condensed matter physics community to use entanglement entropy as a probe of new physics of experimental relevance. Indeed, we have found that the entanglement entropy is a very sharp probe of the physics at the transition temperature , the ground state of the system at , and also at intermediate temperatures, where, in mapping out the full temperature range, we identified a novel^{6}^{6}6Note that while jumps in the entanglement entropy for gravity duals have been observed elsewhere in the literature (see e.g. refs. [5, 30, 31]), our cases here (and in ref. [27]) are crucially qualitatively different from those cases since our kink in the entropy function does not result from a change in topology in the relevant minimal surfaces, but instead arise from a multivaluedness in the entropy from contributions of minimal surfaces of the same topology. transition in the entropy. Some of the novel physics (arising from multiple extremal solutions for the entropy at a given point in parameter space) recalled phenomena observed in our earlier studies of the time evolution of entanglement entropy [27]. The origins of the transition from a field theory perspective would be very interesting to study, and we leave that for future work. It would also be of value to study the fate of the physics away from the strict large limit we have been working in here.

The study presented here also served as another holographic example of the behaviour of entanglement entropy along an RG flow, which we studied in ref. [26], and in fact we were able to confirm some more of our predictions from that paper using phenomena observed here.

We expect that this is just the beginning of a series of fruitful investigations of this type, shedding more light on a wide variety of strongly coupled quantum phenomena of interest.

## Acknowledgements

TA and CVJ would like to thank the US Department of Energy for support under grant DE-FG03-84ER-40168, and Nikolay Bobev and Arnab Kundu for conversations and correspondence. We thank Jerome Gauntlett for helpful comments on an earlier version of this manuscript that led us to clarify some remarks concerning stability. TA is also supported by the USC Dornsife College of Letters, Arts and Sciences.

## References

- [1] S. Ryu and T. Takayanagi, Holographic derivation of entanglement entropy from AdS/CFT, Phys.Rev.Lett. 96 (2006) 181602, [hep-th/0603001].
- [2] S. Ryu and T. Takayanagi, Aspects of holographic entanglement entropy, JHEP 08 (2006) 045, [hep-th/0605073].
- [3] S. N. Solodukhin, Entanglement entropy of black holes and AdS/CFT correspondence, Phys. Rev. Lett. 97 (2006) 201601, [hep-th/0606205].
- [4] T. Hirata and T. Takayanagi, AdS/CFT and strong subadditivity of entanglement entropy, JHEP 02 (2007) 042, [hep-th/0608213].
- [5] T. Nishioka and T. Takayanagi, AdS bubbles, entropy and closed string tachyons, JHEP 01 (2007) 090, [hep-th/0611035].
- [6] M. Headrick and T. Takayanagi, A holographic proof of the strong subadditivity of entanglement entropy, Phys. Rev. D76 (2007) 106013, [arXiv:0704.3719].
- [7] S. N. Solodukhin, Entanglement entropy, conformal invariance and extrinsic geometry, Phys. Lett. B665 (2008) 305–309, [arXiv:0802.3117].
- [8] H. Casini, M. Huerta, and L. Leitao, Entanglement entropy for a Dirac fermion in three dimensions: vertex contribution, Nucl. Phys. B814 (2009) 594–609, [arXiv:0811.1968].
- [9] T. Nishioka, S. Ryu, and T. Takayanagi, Holographic Entanglement Entropy: An Overview, J. Phys. A42 (2009) 504008, [arXiv:0905.0932].
- [10] H. Casini, M. Huerta, and R. C. Myers, Towards a derivation of holographic entanglement entropy, JHEP 1105 (2011) 036, [arXiv:1102.0440].
- [11] J. M. Maldacena, The large n limit of superconformal field theories and supergravity, Adv. Theor. Math. Phys. 2 (1998) 231–252, [hep-th/9711200].
- [12] S. S. Gubser, I. R. Klebanov, and A. M. Polyakov, Gauge theory correlators from non-critical string theory, Phys. Lett. B428 (1998) 105–114, [hep-th/9802109].
- [13] E. Witten, Anti-de sitter space and holography, Adv. Theor. Math. Phys. 2 (1998) 253–291, [hep-th/9802150].
- [14] E. Witten, Anti-de sitter space, thermal phase transition, and confinement in gauge theories, Adv. Theor. Math. Phys. 2 (1998) 505–532, [hep-th/9803131].
- [15] S. A. Hartnoll, C. P. Herzog, and G. T. Horowitz, Holographic Superconductors, JHEP 12 (2008) 015, [arXiv:0810.1563].
- [16] S. A. Hartnoll, C. P. Herzog, and G. T. Horowitz, Building a Holographic Superconductor, Phys. Rev. Lett. 101 (2008) 031601, [arXiv:0803.3295].
- [17] J. P. Gauntlett, J. Sonner, and T. Wiseman, Holographic superconductivity in M-Theory, arXiv:0907.3796.
- [18] S. S. Gubser and I. Mitra, Instability of charged black holes in Anti-de Sitter space, hep-th/0009126.
- [19] N. Bobev, N. Halmagyi, K. Pilch, and N. P. Warner, Supergravity Instabilities of Non-Supersymmetric Quantum Critical Points, Class.Quant.Grav. 27 (2010) 235013, [arXiv:1006.2546].
- [20] D. Cassani and P. Koerber, Tri-Sasakian consistent reduction, JHEP 1201 (2012) 086, [arXiv:1110.5327].
- [21] N. Bobev, A. Kundu, K. Pilch, and N. P. Warner, Minimal Holographic Superconductors from Maximal Supergravity, JHEP 1203 (2012) 064, [arXiv:1110.3454].
- [22] S. S. Gubser, C. P. Herzog, S. S. Pufu, and T. Tesileanu, Superconductors from Superstrings, arXiv:0907.3510.
- [23] O. Aharony, S. S. Gubser, J. M. Maldacena, H. Ooguri, and Y. Oz, Large n field theories, string theory and gravity, Phys. Rept. 323 (2000) 183–386, [hep-th/9905111].
- [24] P. Basu, A. Mukherjee, and H.-H. Shieh, Supercurrent: Vector Hair for an AdS Black Hole, Phys.Rev. D79 (2009) 045010, [arXiv:0809.4494].
- [25] C. Herzog, P. Kovtun, and D. Son, Holographic model of superfluidity, Phys.Rev. D79 (2009) 066002, [arXiv:0809.4870]. 17 pages, 4 figures/ v2 ref added.
- [26] T. Albash and C. V. Johnson, Holographic Entanglement Entropy and Renormalization Group Flow, JHEP 1202 (2012) 095, [arXiv:1110.1074]. 25 pages. 12 Figures. Corrected minor typos and clarified certain results.
- [27] T. Albash and C. V. Johnson, Evolution of Holographic Entanglement Entropy after Thermal and Electromagnetic Quenches, New J.Phys. 13 (2011) 045017, [arXiv:1008.3027].
- [28] V. Balasubramanian, A. Bernamonti, J. de Boer, N. Copland, B. Craps, et. al., Holographic Thermalization, Phys.Rev. D84 (2011) 026010, [arXiv:1103.2683].
- [29] R. C. Myers and A. Singh, Comments on Holographic Entanglement Entropy and RG Flows, JHEP 1204 (2012) 122, [arXiv:1202.2068]. References added.
- [30] I. R. Klebanov, D. Kutasov, and A. Murugan, Entanglement as a probe of confinement, Nucl.Phys. B796 (2008) 274–293, [arXiv:0709.2140].
- [31] A. Pakman and A. Parnachev, Topological Entanglement Entropy and Holography, JHEP 0807 (2008) 097, [arXiv:0805.1891].