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Holographic Entanglement Negativity for Adjacent Subsystems in AdSd+1/CFTd\mathrm{AdS_{d+1}/CFT_{d}}

Parul Jain E-mail:  parul.jain@ca.infn.it Dipartimento di Fisica, Università di Cagliari
Cittadella Universitaria, 09042 Monserrato, Italy
INFN, Sezione di Cagliari,Italy
Department of Physics
Indian Institute of Technology
Kanpur, 208016
India
Vinay Malvimat E-mail:  vinaymm@iitk.ac.in Department of Physics
Indian Institute of Technology
Kanpur, 208016
India
Sayid Mondal E-mail:  sayidphy@iitk.ac.in Department of Physics
Indian Institute of Technology
Kanpur, 208016
India
Gautam Sengupta E-mail:  sengupta@iitk.ac.in Department of Physics
Indian Institute of Technology
Kanpur, 208016
India

1 Introduction

Quantum entanglement has developed into an ubiquitous feature of modern fundamental physics in recent times connecting a spectrum of diverse areas from condensed matter physics to quantum gravity. In this regard entanglement entropy has evolved as the most significant and convenient measure to characterize the entanglement of a bipartite quantum system in a pure state. From quantum information theory this is defined as the von Neumann entropy of the reduced density matrix of the corresponding subsystem. For (1+1)(1+1)-dimensional conformal field theories (CFT1+1CFT_{1+1}) the entanglement entropy may be computed through the replica technique developed by Calabrese et al in [1, 2].

In the context of the AdS/CFTAdS/CFT correspondence, Ryu and Takayanagi in [3, 4] proposed a prescription to compute the entanglement entropy of holographic CFTCFTs. For a subsystem described by a spatial region AA on the boundary the entanglement entropy is given from this conjecture by the area of the co-dimension two bulk AdSd+1AdS_{d+1} extremal surface anchored on the region AA. In the recent past this has led to intense research activity into entanglement issues for diverse holographic CFTCFTs both at zero and finite temperatures [5, 6, 7, 8, 9, 10, 11].

Although the entanglement entropy was crucial for the characterization of entanglement for bipartite systems in pure states, it was inadequate as an entanglement measure for mixed quantum states. In a seminal work Vidal and Werner [12] introduced a quantity termed entanglement negativity as a computable measure for the upper bound on the distillable entanglement in mixed states. The non convexity property of this entanglement measure was subsequently established in [13]. Interestingly, the authors in [14, 15, 16] computed this quantity in CFT1+1{CFT_{1+1}} employing a variant of the usual replica technique involving a certain four point function of the twist/anti-twist fields. This technique has been extensively employed to compute the entanglement negativity of various mixed state configurations in CFT1+1CFT_{1+1}[17, 18, 19, 20, 21, 22].

Naturally, it was critical to establish a holographic description for the entanglement negativity of boundary CFTCFTs in terms of the bulk dual geometry in the AdS/CFTAdS/CFT scenario. In spite of interesting insights in [23, 24], a clear holographic prescription for the entanglement negativity of CFTCFTs remained an unresolved issue. Two of the present authors (VM and GS) in the articles [25, 26, 27] (CMS) proposed a holographic conjecture for the entanglement negativity of such boundary CFTdCFT_{d}s which exactly reproduced the CFT1+1CFT_{1+1} [16] results in the large central charge limit.

It is important to emphasize that the CMS conjecture mentioned above refers to the entanglement negativity of a single subsystem within an infinite system described by the boundary CFTdCFT_{d}. In the articles [15, 16], the authors computed the entanglement negativity of a mixed state characterized by two finite intervals A1A_{1} and A2A_{2} in a CFT1+1CFT_{1+1} both at zero and finite temperatures. In a recent communication [28], the present authors established an independent holographic conjecture for the entanglement negativity between the two intervals mentioned above in the context of AdS3/CFT2AdS_{3}/CFT_{2}. It was shown there that the corresponding entanglement negativity was characterized by a certain algebraic sum of the geodesic lengths in the bulk AdS3AdS_{3} space time anchored on the two adjacent intervals, which reduced to the holographic mutual information. Remarkably the holographic entanglement negativity computed from the above prescription exactly reproduced the CFT1+1CFT_{1+1} results both for zero and finite temperatures in the large central charge limit [15, 29]. The holographic conjecture for the entanglement negativity [28] alluded above allowed a direct generalization to the AdSd+1/CFTdAdS_{d+1}/CFT_{d} scenario. In this case the entanglement negativity could be characterized in terms of an algebraic sum of the areas of bulk co-dimension two extremal surfaces anchored on the respective subsystems in the boundary CFTdCFT_{d}. As earlier this reduces to the holographic mutual information between the subsystems.

In this article we provide the first non trivial higher dimensional examples in the context of the AdSd+1/CFTdAdS_{d+1}/CFT_{d} correspondence to establish the efficacy of our conjecture. To this end we consider the mixed state of two adjacent subsystems A1A_{1} and A2A_{2} characterized by rectangular strip geometries and compute the corresponding holographic entanglement negativity in CFTdCFT_{d}s at both zero and finite temperatures. For zero temperature the bulk configuration is described by the AdSd+1AdS_{d+1} vacuum whereas the finite temperature scenario is described by the AdSd+1AdS_{d+1}-Schwarzschild black hole. For the finite temperature case the computation of the holographic entanglement negativity requires both a low and a high temperature approximations for the areas of the corresponding bulk extremal surfaces. At low temperatures the leading contribution arises from the AdSd+1AdS_{d+1} vacuum corrected by sub leading thermal contributions. Interestingly for the high temperature case on the other hand the thermal contribution are precisely subtracted out. Hence at the leading order the entanglement negativity at high temperature is characterized by the area of the entangling surface on the boundary.

This article is organized as follows, in section 22 we briefly review the computation of the holographic entanglement negativity of two adjacent intervals in the AdS3/CFT2AdS_{3}/CFT_{2} scenario described in [28]. In section 33 we establish the corresponding holographic conjecture for the entanglement negativity of two adjacent subsystems in the context of the AdSd+1/CFTdAdS_{d+1}/CFT_{d} correspondence. In the subsequent section 44 we employ our conjecture to compute the holographic entanglement negativity for two adjacent subsystems of rectangular strip geometries at zero temperature from the bulk AdSd+1AdS_{d+1} vacuum. In section 55 we describe the corresponding computation for the finite temperature scenario from a bulk AdSd+1AdS_{d+1}-Schwarzschild black hole. In the final section 66 we summarize our results and present our conclusions and future open issues.

2 Entanglement negativity in CFT1+1\mathrm{CFT_{1+1}}

In this section, we briefly recapitulate the essential elements for the entanglement negativity of mixed states in a CFT1+1CFT_{1+1}  [14, 15]. To this end we consider a tripartition in the CFT1+1CFT_{1+1} described by the spatial intervals A1A_{1}, A2A_{2} and BB with A=A1A2=[u1,v1][u2,v2]A=A_{1}\cup A_{2}=[u_{1},v_{1}]\cup[u_{2},v_{2}], and B=AcB=A^{c} represents the rest of the system111Note that the definition of entanglement negativity requires the concept of purification which involves embedding the given bipartite system (A1A2=AA_{1}\cup A_{2}=A) in a mixed state, inside a larger system BB such that the full system A1A2BA_{1}\cup A_{2}\cup B is in a pure quantum state. The larger system BB is then traced out to obtain the required mixed state ρA\rho_{A} of the bipartite quantum system. . The reduced density matrix of the subsystem AA is defined as ρA=TrBρ\rho_{A}=\mathrm{Tr}_{B}~\rho and ρAT2\rho_{A}^{T_{2}} is the partial transpose of the reduced density matrix with respect to the interval A2A_{2}. The entanglement negativity  \mathcal{E} is defined as the logarithm of the trace norm of the partially transposed reduced density matrix [12], which is expressed as

=lnTr|ρAT2|.\mathcal{E}=\ln\mathrm{Tr}|\rho_{A}^{T_{2}}|. (2.1)

The entanglement negativity may now be obtained through a replica technique as discussed in [14, 15] to determine Tr(ρAT2)ne\mathrm{Tr}~(\rho_{A}^{T_{2}})^{n_{e}} and the replica limit is given as the analytic continuation of nen_{e} through even sequences to ne1n_{e}\to 1. This leads to the following expression for the entanglement negativity

=limne1lnTr(ρAT2)ne.\mathcal{E}=\lim_{n_{e}\rightarrow 1}\ln\mathrm{Tr}(\rho_{A}^{T_{2}})^{n_{e}}. (2.2)

For the mixed state described by the two intervals as shown in Fig. (1), the quantity Tr(ρAT2)ne\mathrm{Tr}(\rho_{A}^{T_{2}})^{n_{e}} is given by a four point function of the twist operators on the complex plane from the replica technique described in [14, 15], as follows

Tr(ρAT2)ne=𝒯ne(u1)𝒯¯ne(v1)𝒯¯ne(u2)𝒯ne(v2).\mathrm{Tr}(\rho_{A}^{T_{2}})^{n_{e}}=\langle\mathcal{T}_{n_{e}}(u_{1})\overline{\mathcal{T}}_{n_{e}}(v_{1})\overline{\mathcal{T}}_{n_{e}}(u_{2})\mathcal{T}_{n_{e}}(v_{2})\rangle_{\mathbb{C}}. (2.3)
BBBA1A_{1}l1l_{1}u1u_{1}v1v_{1}A2A_{2}l2l_{2}u2u_{2}v2v_{2}
Figure 1: Schematic of two disjoint intervals A1A_{1} and A2A_{2} in a (1+1)(1+1)-dimensional boundary CFT\mathrm{CFT}.

2.1 Entanglement negativity for two adjacent intervals in vacuum

We first review the computation of the entanglement negativity for the mixed state of two adjacent intervals in a CFT1+1CFT_{1+1} at zero temperature [14, 15] and the corresponding holographic description in [28]. The related configuration may now be obtained by setting v1u2v_{1}\rightarrow u_{2} with u2=0,u1=l1u_{2}=0,~u_{1}=-l_{1} and v2=l2v_{2}=l_{2} as shown in Fig. (2) described below.

BBu1u_{1}u2u_{2}v2v_{2}A1A_{1}l1l_{1}A2A_{2}l2l_{2}
Figure 2: Schematic of two adjacent intervals A1A_{1} and A2A_{2} in a (1+1)(1+1)-dimensional CFT\mathrm{CFT}.

The quantity Tr(ρAT2)ne\mathrm{Tr}(\rho_{A}^{T_{2}})^{n_{e}} in the eq. (2.3) for the two adjacent intervals is now described by a three point function of the twist operators as follows

Tr(ρAT2)ne=𝒯ne(l1)𝒯¯ne2(0)𝒯ne(l2).\mathrm{Tr}(\rho_{A}^{T_{2}})^{n_{e}}=\langle\mathcal{T}_{n_{e}}(-l_{1})\overline{\mathcal{T}}^{2}_{n_{e}}(0)\mathcal{T}_{n_{e}}(l_{2})\rangle. (2.4)

The replica limit ne1n_{e}\to 1 on eq. (2.4) now leads to the following expression for the entanglement negativity

=c4ln(l1l2(l1+l2)a)+const,\mathcal{E}=\frac{c}{4}\ln\Big{(}\frac{l_{1}l_{2}}{(l_{1}+l_{2})a}\Big{)}+\mathrm{const}, (2.5)

where aa is the UV cutoff for the CFTCFT. The ‘const’ term in the above expression may be neglected in the large central charge limit ( see discussion below) [29, 28].

In [28] the present authors demonstrated that the universal part of the three point function in eq.(2.4) is dominant in the large central charge limit and factorizes into two point correlation functions. Employing the geodesic approximation for these two point functions from the standard AdS/CFTAdS/CFT dictionary then leads us to a holographic conjecture for the entanglement negativity of the configuration described above. In the context of the AdS3/CFT2AdS_{3}/CFT_{2} scenario, the holographic conjecture may be expressed as follows

=316GN(3)(A1+A2A1A2).\mathcal{E}=\frac{3}{16G^{(3)}_{N}}(\mathcal{L}_{A_{1}}+\mathcal{L}_{A_{2}}-\mathcal{L}_{A_{1}\cup A_{2}}). (2.6)

Here GN(3)G^{(3)}_{N} is the (2+1)(2+1)-dimensional Newton constant and Ai\mathcal{L}_{A_{i}} is the geodesic length anchored on the interval AiA_{i}. Using the Ryu-Takayanagi conjecture [4, 3] the eq. (2.6) reduces to the following

=34(SA1+SA2SA1A2)=34[(A1,A2)],\mathcal{E}=\frac{3}{4}(S_{A_{1}}+S_{A_{2}}-S_{A_{1}\cup A_{2}})=\frac{3}{4}[{\cal I}(A_{1},A_{2})], (2.7)

which is precisely the mutual information between the subsystems described by the intervals A1A_{1} and A2A_{2}. Note that the entanglement negativity is a measure of the upper bound on the distillable entanglement of the bipartite system whereas the mutual information is the upper bound on the total correlations between the subsystems. Therefore they are measures of distinct quantities in quantum information theory. However the universal parts of both are dominant in the large central charge limit and admit a holographic description which match exactly for this particular mixed state configuration 222Note that recently this matching between the universal parts of entanglement negativity and mutual information for the adjacent interval case has also been observed in both local and global quench problems in a CFT1+1CFT_{1+1} [30, 20]. . Note that the full entanglement negativity and the mutual information involve non universal terms which are sub leading in 1c\frac{1}{c} in the holographic ( large central charge) limit as described below.

We would like to emphasize here that the exact relation between the holographic negativity and the holographic mutual information described by eq.(2.7) is valid only for this specific mixed state configuration of adjacent intervals and is not expected to hold for generic mixed states. However it could be shown in [25, 26] that for a bipartite mixed state involving a single interval the holographic entanglement negativity was described by a sum of specific holographic mutual informations between subsystems relevant to the purification. Hence there seems to be a relation between these two measures in the holographic limit whose specific nature depends on the mixed state configuration in question. A quantum information theoretic understanding of this phenomena is an open issue which needs elucidation.

In the AdS3/CFT2AdS_{3}/CFT_{2} scenario being considered here, the bulk dual of the CFT1+1CFT_{1+1} at zero temperature is described by the AdS3AdS_{3} vacuum, whose metric is given as follows

ds2=(r2R2)dt2+(r2R2)1dr2+(r2R2)dϕ2,ds^{2}=-\left(\frac{r^{2}}{R^{2}}\right)dt^{2}+\left(\frac{r^{2}}{R^{2}}\right)^{-1}dr^{2}+\left(\frac{r^{2}}{R^{2}}\right)d\phi^{2}, (2.8)

where RR is the radius of the AdS3\mathrm{AdS_{3}} space time. Employing the conjecture described above [28] the holographic entanglement negativity of the configuration in Fig. (2) may now be obtained as

=3R8GN(3)ln(l1l2(l1+l2)a).\mathcal{E}=\frac{3R}{8G^{(3)}_{N}}\ln\Big{(}\frac{l_{1}l_{2}}{(l_{1}+l_{2})a}\Big{)}. (2.9)

Remarkably the holographic entanglement negativity exactly reproduces the CFT1+1CFT_{1+1} result given in eq. (2.5) in the large central charge limit [29, 28] upon using the Brown-Henneaux formula c=3R2GN(3){c}=\frac{3R}{2G^{(3)}_{N}} [31].

Note that here we have utilized the relation r01ar_{0}\sim\frac{1}{a} from the AdS/CFTAdS/CFT dictionary that connects the UV cut-off for the boundary CFT1+1CFT_{1+1} to the bulk infra red cut-off (r0r_{0}) ( to regulate the lengths of geodesics in eq.(2.6) ). The eq.(2.9) suggests that only the leading universal part of the negativity in eq.(2.5) is captured by our conjecture whereas the non-universal constant term is sub leading in the large central charge limit. However the precise renormalization procedure for this is an open issue as the first term in eq.(2.5) depends on the UV cut-off whereas the non-universal part is a constant. We mention here that the same issue also occurs in the Ryu-Takayanagi conjecture for the holographic entanglement entropy of a single interval in a CFT1+1CFT_{1+1} where the non-universal part is once again a constant (see also [32, 33, 34] for related discussions on renormalized entanglement entropy in higher dimensions). In contrast for higher point twist correlators in a CFT1+1CFT_{1+1} relevant to both the entanglement entropy and the entanglement negativity for multiple intervals involve non universal functions ( of the cross ratios). In this case using monodromy techniques it was clearly demonstrated that the universal parts which admit a bulk geometrical description, are dominant in the large central charge limit [35, 36] whereas the non universal functions are sub leading in 1c\frac{1}{c}.

2.2 Entanglement negativity for two adjacent intervals at finite temperature

For the finite temperature case the entanglement negativity for the mixed state described by the configuration in Fig. (2) in the context of CFT1+1CFT_{1+1} may be obtained from eq. (2.4) through the conformal map zw=β2πlnzz\rightarrow w=\frac{\beta}{2\pi}~\ln z to the cylinder of circumference β\beta. This leads to the following expression for the entanglement negativity

=c4ln(βπasinh(πl1β)sinh(πl2β)(sinhπ(l1+l2)β))+const,\mathcal{E}=\frac{c}{4}\ln\Bigg{(}\frac{\beta}{\pi a}\frac{\sinh(\frac{\pi l_{1}}{\beta})\sinh(\frac{\pi l_{2}}{\beta})}{(\sinh\frac{\pi(l_{1}+l_{2})}{\beta})}\Bigg{)}+\mathrm{const}, (2.10)

where β=1/T\beta=1/T and aa are the inverse temperature and the UV cut-off in the boundary field theory respectively. As earlier in the large central charge limit the ’const’ term in the above equation may be neglected [29, 28].

The bulk dual for the above case is described by the (2+1)(2+1) dimensional Euclidean BTZ black hole whose metric is

ds2=(r2r+2)R2dτ2+R2(r2r+2)dr2+r2R2dϕ2.ds^{2}=\frac{\left(r^{2}-r_{+}^{2}\right)}{R^{2}}d\tau^{2}+\frac{R^{2}}{\left(r^{2}-r_{+}^{2}\right)}dr^{2}+\frac{r^{2}}{R^{2}}d\phi^{2}. (2.11)

Here the horizon radius r+r_{+} is related to the inverse Hawking temperature as β=2πR2/r+\beta=2\pi R^{2}/r_{+}. The holographic entanglement negativity for the two adjacent intervals at a finite temperature may then be obtained from the conjecture eq. (2.6) proposed in [28]. Interestingly as earlier this exactly reproduces the finite temperature CFT1+1CFT_{1+1} result given by eq. (2.10) in the large central charge limit upon using the Brown-Henneaux formula.

3 Holographic entanglement negativity for AdSd+1/CFTd\mathrm{AdS_{d+1}/CFT_{d}}

In this section we establish the holographic entanglement negativity conjecture for a mixed state described by two adjacent subsystems in a boundary CFTdCFT_{d} in the context of the AdSd+1/CFTdAdS_{d+1}/CFT_{d} scenario which was alluded to in the article [28]. As mentioned in the Introduction this would involve an algebraic sum of the areas of the bulk co-dimension two extremal surfaces anchored on the respective subsystems. From the conjecture described in [28] the holographic entanglement negativity may then be expressed as follows

=316GN(d+1)(𝒜1+𝒜2𝒜12),\mathcal{E}=\frac{3}{16G^{(d+1)}_{N}}\big{(}\mathcal{A}_{1}+\mathcal{A}_{2}-\mathcal{A}_{12}\big{)}, (3.1)

where 𝒜i\mathcal{A}_{i} is the extremal area of the co-dimension two surface anchored on the subsystem AiA_{i}. Using the Ryu-Takayanagi prescription [4, 3], it is possible to express the holographic entanglement negativity in the following form

=34(SA1+SA2SA1A2)=34[(A1,A2)],\mathcal{E}=\frac{3}{4}(S_{A_{1}}+S_{A_{2}}-S_{A_{1}\cup A_{2}})=\frac{3}{4}[{\cal I}(A_{1},A_{2})], (3.2)

where SAiS_{A_{i}} is the holographic entanglement entropy of the subsystem AiA_{i}. Interestingly the expression in eq. (3.2) is the holographic mutual information between the two adjacent subsystems modulo a constant factor. We are now ready to employ our holographic conjecture to evaluate the entanglement negativity for two adjacent subsystems described by (d1)(d-1)-dimensional spatial rectangular strip geometries in the boundary CFTdCFT_{d} which we will describe in the subsequent sections.

4 Holographic entanglement negativity for AdSd+1/CFTd\mathrm{AdS_{d+1}/CFT_{d}} in vacuum

As mentioned above in this section we now proceed to the computation of the holographic entanglement negativity for two adjacent subsystems described by rectangular strip geometries in the boundary CFTdCFT_{d} at zero temperature. The corresponding bulk dual geometry in this case is the AdSd+1AdS_{d+1} vacuum space time whose metric in the Poincare coordinates is given as

ds2=1z2(dt2+i=1d1dxi2+dz2),ds^{2}=\frac{1}{z^{2}}\Big{(}-dt^{2}+\sum_{i=1}^{d-1}dx_{i}^{2}+dz^{2}\Big{)}, (4.1)

where the AdSAdS radius has been set to R=1R=1. The respective rectangular strip geometries of the two subsystems A1A_{1} and A2A_{2} depicted in Fig. (3) are then specified as follows

x=x1[lj2,lj2]xi=[L2,L2],i=2,,(d1),j=1,2.x=x^{1}\equiv[-\frac{l_{j}}{2},\frac{l_{j}}{2}]~~x^{i}=[-\frac{L}{2},\frac{L}{2}],~~i=2,...,(d-1),~~j=1,2. (4.2)
Refer to caption
Figure 3: Schematic of the extremal surfaces that are anchored on the subsystems A1A_{1}, A2A_{2} and A1A2A_{1}\cup A_{2} involved in the computation of the holographic entanglement negativity of the adjacent subsystems in the boundary CFTd\mathrm{CFT}_{d}.

We now briefly describe the computation for the areas of bulk co-dimension two extremal surfaces anchored on rectangular strip geometries in the boundary CFTdCFT_{d} [4]. The corresponding area functional is expressed in the following way

𝒜=Ld2l/2l/2𝑑x1+(dzdx)2zd1.{\cal A}=L^{d-2}\int_{-l/2}^{l/2}dx\frac{\sqrt{1+(\frac{dz}{dx})^{2}}}{z^{d-1}}. (4.3)

The Euler-Lagrange equation for the extremization problem is then given as

dzdx=z2(d1)z2(d1)zd1,\frac{dz}{dx}=\frac{\sqrt{z_{*}^{2(d-1)}-z^{2(d-1)}}}{z^{d-1}}, (4.4)

where z=zz=z_{*} is the turning point of the extremal surface. The extremal area may then be described as

𝒜=2d2(La)d22I(Lz)d2,\mathcal{A}=\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2}-2I\Big{(}\frac{L}{z_{*}}\Big{)}^{d-2}, (4.5)

where aa is the UV cutoff and the constant II is given as

I=1d201dyyd1(11y2(d1)1)=πΓ(2d2(d1))Γ(12(d1)).I=\frac{1}{d-2}-\int_{0}^{1}\frac{dy}{y^{d-1}}\Big{(}\frac{1}{\sqrt{1-y^{2(d-1)}}}-1\Big{)}=-\frac{\sqrt{\pi}~\Gamma\Big{(}\frac{2-d}{2(d-1)}\Big{)}}{\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}. (4.6)

Using the eq.(4.4), eq. (4.5) and eq. (4.6) it is now possible to express the area of the extremal co-dimension two surface as

𝒜=𝒜divs0(Ll)d2,{\cal A}={\cal A}_{div}-s_{0}~\Big{(}\frac{L}{l}\Big{)}^{d-2}, (4.7)

where the divergent part of the area 𝒜div{\cal A}_{div} and the constant s0s_{0} are given as

s0\displaystyle s_{0} =2d1π(d1)/2d2(Γ(d2(d1))Γ(12(d1)))d1,\displaystyle=\frac{2^{d-1}\pi^{(d-1)/2}}{d-2}\Bigg{(}\frac{\Gamma(\frac{d}{2(d-1)})}{\Gamma(\frac{1}{2(d-1)})}\Bigg{)}^{d-1}, (4.8)
𝒜div\displaystyle{\cal A}_{div} =2d2(La)d2.\displaystyle=\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2}.

One may now determine the holographic entanglement negativity \mathcal{E} for the mixed state at zero temperature in the boundary CFTdCFT_{d} described by the two strip geometries in Fig. (3) to be as follows

=\displaystyle\mathcal{E}= 316GN(d+1)[2d2(La)d2s0{(Ll1)d2+(Ll2)d2(Ll1+l2)d2}].\displaystyle\frac{3}{16G_{N}^{(d+1)}}\Bigg{[}\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2}-s_{0}\bigg{\{}\Big{(}\frac{L}{l_{1}}\Big{)}^{d-2}+\Big{(}\frac{L}{l_{2}}\Big{)}^{d-2}-\Big{(}\frac{L}{l_{1}+l_{2}}\Big{)}^{d-2}\bigg{\}}\Bigg{]}. (4.9)

The first term in the above expression is the divergent term which is proportional to the area of the entangling surface between the two spatial strips on the dd dimensional boundary and the second term describes the finite part of the negativity.

5 Holographic entanglement negativity for AdSd+1/CFTd\mathrm{AdS_{d+1}/CFT_{d}} at finite temperature

At finite temperatures the boundary CFTdCFT_{d} is dual to the AdSd+1AdS_{d+1}-Schwarzschild black hole with the following metric where the AdSAdS-radius has been set to R=1R=1

ds2=r2(1rhdrd)dt2+dr2r2(1rhdrd)+r2dx2.ds^{2}=-r^{2}\Big{(}1-\frac{r_{h}^{d}}{r^{d}}\Big{)}dt^{2}+\frac{dr^{2}}{r^{2}\Big{(}1-\frac{r_{h}^{d}}{r^{d}}\Big{)}}+r^{2}d\vec{x}^{2}. (5.1)

The horizon radius rhr_{h} is related to the Hawking temperature as T=rhd/4πT=r_{h}d/4\pi and x(x,xi)\vec{x}\equiv(x,x^{i}) are the coordinates on the boundary. We first briefly review the computation for the area 𝒜{\cal A} of the bulk AdSd+1AdS_{d+1} co-dimension two extremal surface anchored on a single rectangular strip on the boundary as described in [9]. This will be subsequently employed to compute the holographic entanglement negativity for the configuration Fig. (3) in question. The extremal area functional anchored on a single rectangular strip is given as

𝒜=Ld2𝑑rrd2r2x2+1r2(1rhdrd).{\cal A}=L^{d-2}\int drr^{d-2}\sqrt{r^{2}x^{\prime 2}+\frac{1}{r^{2}(1-\frac{r_{h}^{d}}{r^{d}})}}. (5.2)

The corresponding Euler-Lagrange equation for the extremization problem leads to the following

l2=1rc01ud1du(1u2d2)(1rhdrcdud)12,u=rcr,\frac{l}{2}=\frac{1}{r_{c}}\int^{1}_{0}\frac{u^{d-1}du}{\sqrt{(1-u^{2d-2})}}(1-\frac{r_{h}^{d}}{r_{c}^{d}}u^{d})^{-\frac{1}{2}},~~~u=\frac{r_{c}}{r}, (5.3)

where rcr_{c} as earlier describes the turning point. The area functional in terms of the variable uu may now be expressed as follows

𝒜=2Ld2rcd201duud1(1u2d2)(1rhdrcdud)12.{\cal A}=2L^{d-2}r_{c}^{d-2}\int^{1}_{0}\frac{du}{u^{d-1}\sqrt{(1-u^{2d-2})}}(1-\frac{r_{h}^{d}}{r_{c}^{d}}u^{d})^{-\frac{1}{2}}. (5.4)

This leads us to the final expression for the area functional as

𝒜=(𝒜div+𝒜finite),{\cal A}=\big{(}\mathcal{A}_{div}+\mathcal{A}_{finite}\big{)}, (5.5)

where 𝒜div\mathcal{A}_{div} is the temperature independent divergent part and 𝒜finite\mathcal{A}_{finite} is the finite part. These may be expressed as follows

𝒜div=2d2(La)d2,𝒜finite=2Ld2rcd2[πΓ(d22(d1))2(d1)Γ(12(d1))+n=1(12(d1))Γ(n+12)Γ(d(n1)+22(d1))Γ(1+n)Γ(dn+12(d1))(rhrc)nd].\displaystyle\begin{split}\mathcal{A}_{div}&=\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2},\\ \mathcal{A}_{finite}&=2L^{d-2}r_{c}^{d-2}\Bigg{[}\frac{\sqrt{\pi}\Gamma\Big{(}-\frac{d-2}{2(d-1)}\Big{)}}{2(d-1)\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}+\sum_{n=1}^{\infty}\Big{(}\frac{1}{2(d-1)}\Big{)}\frac{\Gamma\Big{(}n+\frac{1}{2}\Big{)}\Gamma\Big{(}\frac{d(n-1)+2}{2(d-1)}\Big{)}}{\Gamma\big{(}1+n\big{)}\Gamma\Big{(}\frac{dn+1}{2(d-1)}\Big{)}}\Big{(}\frac{r_{h}}{r_{c}}\Big{)}^{nd}\Bigg{]}.\end{split} (5.6)

Note that rc>rhr_{c}>r_{h} from [37] ensuring the convergence of the series in 𝒜finite\mathcal{A}_{finite}. The holographic entanglement negativity for the mixed state described by the two intervals in the boundary CFTdCFT_{d} ( Fig. (3) ) may then be obtained from our conjecture eq. (3.1) as

=316GN(d+1)[2d2(La)d2+2Ld2rc1d2{πΓ(d22(d1))2(d1)Γ(12(d1))+n=1(12(d1))Γ(n+12)Γ(d(n1)+22(d1))Γ(1+n)Γ(dn+12(d1))(rhrc1)nd}+2Ld2rc2d2{πΓ(d22(d1))2(d1)Γ(12(d1))+n=1(12(d1))Γ(n+12)Γ(d(n1)+22(d1))Γ(1+n)Γ(dn+12(d1))(rhrc2)nd}2Ld2rc3d2{πΓ(d22(d1))2(d1)Γ(12(d1))+n=1(12(d1))Γ(n+12)Γ(d(n1)+22(d1))Γ(1+n)Γ(dn+12(d1))(rhrc3)nd}].\begin{split}{\cal E}&=\frac{3}{16G_{N}^{(d+1)}}\Bigg{[}\frac{2}{d-2}(\frac{L}{a})^{d-2}\\ &+2L^{d-2}r_{c1}^{d-2}\bigg{\{}\frac{\sqrt{\pi}\Gamma\Big{(}-\frac{d-2}{2(d-1)}\Big{)}}{2(d-1)\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}+\sum_{n=1}^{\infty}\Big{(}\frac{1}{2(d-1)}\Big{)}\frac{\Gamma\Big{(}n+\frac{1}{2}\Big{)}\Gamma\Big{(}\frac{d(n-1)+2}{2(d-1)}\Big{)}}{\Gamma\big{(}1+n\big{)}\Gamma\Big{(}\frac{dn+1}{2(d-1)}\Big{)}}\Big{(}\frac{r_{h}}{r_{c1}}\Big{)}^{nd}\bigg{\}}\\ &+2L^{d-2}r_{c2}^{d-2}\bigg{\{}\frac{\sqrt{\pi}\Gamma\Big{(}-\frac{d-2}{2(d-1)}\Big{)}}{2(d-1)\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}+\sum_{n=1}^{\infty}\Big{(}\frac{1}{2(d-1)}\Big{)}\frac{\Gamma\Big{(}n+\frac{1}{2}\Big{)}\Gamma\Big{(}\frac{d(n-1)+2}{2(d-1)}\Big{)}}{\Gamma\big{(}1+n\big{)}\Gamma\Big{(}\frac{dn+1}{2(d-1)}\Big{)}}\Big{(}\frac{r_{h}}{r_{c2}}\Big{)}^{nd}\bigg{\}}\\ &-2L^{d-2}r_{c3}^{d-2}\bigg{\{}\frac{\sqrt{\pi}\Gamma\Big{(}-\frac{d-2}{2(d-1)}\Big{)}}{2(d-1)\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}+\sum_{n=1}^{\infty}\Big{(}\frac{1}{2(d-1)}\Big{)}\frac{\Gamma\Big{(}n+\frac{1}{2}\Big{)}\Gamma\Big{(}\frac{d(n-1)+2}{2(d-1)}\Big{)}}{\Gamma\big{(}1+n\big{)}\Gamma\Big{(}\frac{dn+1}{2(d-1)}\Big{)}}\Big{(}\frac{r_{h}}{r_{c3}}\Big{)}^{nd}\bigg{\}}\Bigg{]}.\end{split} (5.7)

Here rc1,rc2,rc3r_{c1},r_{c2},r_{c3} are the turning points of the extremal surfaces in the bulk anchored on the strips A1,A2A_{1},A_{2} and A1A2A_{1}\cup A_{2} on the boundary respectively. It is required to evaluate the quantity rcir_{ci} from the eq. (5.3) in terms of lil_{i} and rhr_{h}. The corresponding integral is not analytically solvable but may be determined perturbatively for low and high temperature approximations described in the following subsections.

5.1 Holographic entanglement negativity in the low temperature limit

At low temperature we have Tl1(rhl1)Tl\ll 1~(r_{h}l\ll 1) and rcr_{c} may be determined perturbatively as an expansion in rhlr_{h}l [9], which leads to the finite part of the area (5.6) as

𝒜finite=s0(Ll)d2[1+s1(rhl)d+O[(rhl)2d]].\mathcal{A}_{finite}=s_{0}\Big{(}\frac{L}{l}\Big{)}^{d-2}\bigg{[}1+s_{1}(r_{h}l)^{d}+O[(r_{h}l)^{2d}]\bigg{]}. (5.8)

Here the constants s0s_{0} is given by the eq. (4.8) and s1s_{1} is given as

s1=Γ(12(d1))d+12d+1πd2Γ(d2(d1))dΓ(d+12(d1))(Γ(1d1)Γ(d22(d1))+21d1(d2)Γ(1+12(d1))π(d+1)).s_{1}=\frac{\Gamma\big{(}\frac{1}{2(d-1)}\big{)}^{d+1}}{2^{d+1}\pi^{\frac{d}{2}}\Gamma\big{(}\frac{d}{2(d-1)}\big{)}^{d}\Gamma\big{(}\frac{d+1}{2(d-1)}\big{)}}\bigg{(}\frac{\Gamma\big{(}\frac{1}{d-1}\big{)}}{\Gamma\big{(}-\frac{d-2}{2(d-1)}\big{)}}+\frac{2^{\frac{1}{d-1}}(d-2)\Gamma\big{(}1+\frac{1}{2(d-1)}\big{)}}{\sqrt{\pi}(d+1)}\bigg{)}. (5.9)

The holographic entanglement negativity at low temperature for the mixed state in the boundary CFTdCFT_{d} described by the configuration in Fig (4) may now be obtained from our conjecture (3.1) and the Eqns (5.8) and (5.9) in the following way

=316GN(d+1)[\displaystyle\mathcal{E}=\frac{3}{16G_{N}^{(d+1)}}\Bigg{[} 2d2(La)d2+s0{(Ll1)d2+(Ll2)d2(Ll1+l2)d2}\displaystyle\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2}+s_{0}\Bigg{\{}\Big{(}\frac{L}{l_{1}}\Big{)}^{d-2}+\Big{(}\frac{L}{l_{2}}\Big{)}^{d-2}-\Big{(}\frac{L}{l_{1}+l_{2}}\Big{)}^{d-2}\Bigg{\}} (5.10)
kl1l2Ld2Td+s0{(Ll1)𝒪(Tl1)2d+(Ll2)𝒪(Tl2)2d}].\displaystyle-k~l_{1}l_{2}L^{d-2}T^{d}+s_{0}\Bigg{\{}\Big{(}\frac{L}{l_{1}}\Big{)}{\cal O}\big{(}Tl_{1}\big{)}^{2d}+\Big{(}\frac{L}{l_{2}}\Big{)}{\cal O}\big{(}Tl_{2}\big{)}^{2d}\Bigg{\}}\Bigg{]}.~~~~~~

Here the constant kk is given as

k=2(4πd)ds0s1.k=2(\frac{4\pi}{d})^{d}~s_{0}s_{1}. (5.11)

Note that the first and the second term in the above expression are temperature independent describing the contribution to the holographic entanglement negativity from the AdSAdS vacuum eq. (4.9). The remaining terms are the finite temperature corrections to the holographic entanglement negativity at low temperatures for the boundary CFTdCFT_{d}.

Refer to caption
Figure 4: Schematic of the extremal surfaces that are anchored on the subsystems A1A_{1}, A2A_{2} and A1A2A_{1}\cup A_{2} in the boundary CFTd\mathrm{CFT}_{d} at low temperatures.

5.2 Holographic entanglement negativity in the high temperature limit

For high temperatures we have Tl1(rhl1)Tl\gg 1~(r_{h}l\gg 1) and in this case it is possible to obtain the quantity rcr_{c} eq. (5.3) in a near horizon expansion in ϵ=(rcrh1)\epsilon=(\frac{r_{c}}{r_{h}}-1) [9] as follows

rc=rh(1+ϵ).r_{c}=r_{h}(1+\epsilon). (5.12)

Here ϵ\epsilon is expressed as

ϵ=C1exp(d(d1)2lrh),\displaystyle\begin{split}\epsilon=&C_{1}\exp(-\sqrt{\frac{d(d-1)}{2}}lr_{h}),\\ \end{split} (5.13)

where the constant C1C_{1} is given as

C1=1dexp[d(d1)2{2πΓ(d2(d1))Γ(12(d1))+2n=1(11+ndΓ(12+n)Γ(d(n+1)2(d1))Γ(1+n)Γ(dn+12(d1))12d(d1)n)}].\displaystyle\begin{split}C_{1}=&\frac{1}{d}\ \exp\Bigg{[}\sqrt{\frac{d(d-1)}{2}}\Bigg{\{}\frac{2\sqrt{\pi}\Gamma\Big{(}\frac{d}{2(d-1)}\Big{)}}{\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}\\ &+2\sum_{n=1}^{\infty}\Bigg{(}\frac{1}{1+nd}\frac{\Gamma\Big{(}\frac{1}{2}+n\Big{)}\Gamma\Big{(}\frac{d(n+1)}{2(d-1)}\Big{)}}{\Gamma\Big{(}1+n\Big{)}\Gamma\Big{(}\frac{dn+1}{2(d-1)}\Big{)}}-\frac{1}{\sqrt{2d(d-1)}~n}\Bigg{)}\Bigg{\}}\Bigg{]}.\end{split} (5.14)

The area of the extremal surface at high temperatures is expressed as

𝒜=2d2(La)d2+(4πd)d1[VTd1+C2d8πATd2C18π2d(d1)ATd2exp{(d1)/2d4πTl}+],\displaystyle\begin{split}\mathcal{A}=&\frac{2}{d-2}\Big{(}\frac{L}{a}\Big{)}^{d-2}+\Big{(}\frac{4\pi}{d}\Big{)}^{d-1}\Bigg{[}V~T^{d-1}+\frac{C_{2}~d}{8\pi}A^{\prime}~T^{d-2}\\ &-\frac{C_{1}}{8\pi}\sqrt{2d(d-1)}~A^{\prime}~T^{d-2}~exp~\Big{\{}-\sqrt{(d-1)/2d}~4\pi Tl\Big{\}}+...\Bigg{]},\end{split} (5.15)

where V=lLd2V=l~L^{d-2} and A=2Ld2A^{\prime}=2L^{d-2} are the volume and area of a single strip respectively . The constant term C2C_{2} is given as

C2=2[π(d1)Γ(d2(d1))(d2)Γ(12(d1))+n=111+nd(d1d(n1)+2)Γ(n+1/2)Γ(d(n+1)2d2)Γ(n+1)Γ(dn+12d2)].\displaystyle\begin{split}C_{2}&=2\Bigg{[}-\frac{\sqrt{\pi}(d-1)\Gamma\Big{(}\frac{d}{2(d-1)}\Big{)}}{(d-2)\Gamma\Big{(}\frac{1}{2(d-1)}\Big{)}}+\sum_{n=1}^{\infty}\frac{1}{1+nd}\Big{(}\frac{d-1}{d(n-1)+2}\Big{)}\frac{\Gamma\Big{(}n+1/2\Big{)}\Gamma\Big{(}\frac{d(n+1)}{2d-2}\Big{)}}{\Gamma\big{(}n+1\big{)}\Gamma\Big{(}\frac{dn+1}{2d-2}\Big{)}}\Bigg{]}.\end{split} (5.16)

The holographic entanglement negativity at high temperatures for the mixed state in the boundary CFTdCFT_{d} described by the configuration in Fig. (5) may then be established from the eq. (5.15) employing our conjecture as follows

=316GN(d+1)2(d2)(Aad2)+316GN(d+1)(4πd)d1[C2d4πATd2C14π2d(d1)ATd2{exp((d1)/2d4πTl1)+exp((d1)/2d4πTl2)exp((d1)/2d4πT(l1+l2))}+],\displaystyle\begin{split}{\cal E}=&\frac{3}{16G_{N}^{(d+1)}}\frac{2}{(d-2)}\Big{(}\frac{A}{a^{d-2}}\Big{)}+\frac{3}{16G_{N}^{(d+1)}}\Big{(}\frac{4\pi}{d}\Big{)}^{d-1}\Bigg{[}\frac{C_{2}~d}{4\pi}A~T^{d-2}\\ &-\frac{C_{1}}{4\pi}\sqrt{2d(d-1)}~A~T^{d-2}~\Bigg{\{}exp~\Big{(}-\sqrt{(d-1)/2d}~4\pi Tl_{1}\Big{)}+exp~\Big{(}-\sqrt{(d-1)/2d}~4\pi Tl_{2}\Big{)}\\ &-exp~\Big{(}-\sqrt{(d-1)/2d}~4\pi T(l_{1}+l_{2})\Big{)}\Bigg{\}}+...\Bigg{]},\end{split} (5.17)

where the ellipsis represent the higher order corrections and A=Ld2A=L^{d-2} is the area of the entangling surface shared by the two adjacent strips on the boundary. Interestingly in the above expression notice that the thermal contribution to the holographic entanglement negativity (proportional to the volume in the eq. (5.15)) has been subtracted out rendering it to be proportional to the area of the entangling surface. This is in conformity with the usual expectations from quantum information theory and furthermore, recently it has been demonstrated that entanglement negativity does obey an area law in various many body systems such as the finite temperature quantum spin model and the two dimensional harmonic lattice in [38, 39].

Refer to caption
Figure 5: Schematic of the extremal surfaces that are anchored on the subsystems A1A_{1}, A2A_{2} and A1A2A_{1}\cup A_{2} in the boundary CFTd\mathrm{CFT}_{d} at high temperatures.

6 Summary and conclusions

To summarize we have established a holographic conjecture for the entanglement negativity for mixed states of adjacent subsystems in zero and finite temperature boundary CFTdCFT_{d}s. The relevant subsystems are described by (d1)(d-1)-dimensional spatial rectangular strip geometries at the boundary in a AdSd+1/CFTdAdS_{d+1}/CFT_{d} scenario. Our conjecture involves a certain algebraic sum of the areas of bulk co dimension two extremal surfaces anchored on the corresponding subsystems on the AdSd+1AdS_{d+1} boundary and was motivated by the corresponding analysis for the AdS3/CFT2AdS_{3}/CFT_{2} scenario in [28]. It is interesting that the algebraic sum described above actually characterizes the holographic mutual information between the two adjacent subsystems. Note that these two measures are completely distinct quantities in quantum information theory. Our conjecture states that only their universal parts (which are dominant in the holographic limit) match upto a numerical factor for the particular mixed state configuration of adjacent subsystems. We emphasize that such a matching between the universal parts of negativity and mutual information of adjacent intervals in a CFT1+1CFT_{1+1} has also been demonstrated for both local and global quench problems in [30, 20].

The holographic entanglement negativity for the boundary CFTdCFT_{d} at zero temperature could then be computed from the bulk dual geometry described by the AdSd+1AdS_{d+1} vacuum from our conjecture. The corresponding holographic entanglement negativity for the boundary CFTdCFT_{d} at finite temperature however involved a bulk dual geometry described by the AdSd+1AdS_{d+1}-Schwarzschild black hole with a planar horizon. In the latter case the area integrals are not analytically solvable and were evaluated in a perturbative expansion for low and high temperatures. It was observed from our computation that the leading contribution to the holographic entanglement negativity at low temperature arises from the AdSd+1AdS_{d+1} vacuum with subleading thermal corrections. Interestingly on the other hand at high temperatures the finite part of the holographic entanglement negativity is proportional to the area of the entangling surface on the boundary whereas the volume dependent thermal parts cancel out. It has been demonstrated that entanglement negativity does obey such area laws in various condensed matter systems confirming the expectation from quantum information theory (See [38, 39]).

Through these examples we demonstrated that our conjecture provides a direct and elegant holographic prescription to compute the entanglement negativity for mixed states described by the specific configuration in boundary CFTdCFT_{d} both at zero and finite temperatures. However for the higher dimensional AdSd+1/CFTdAdS_{d+1}/CFT_{d} scenario this remains a conjecture. So in higher dimensions our conjecture requires further analysis towards a possible proof from the bulk side which remains a non trivial open issue. In this context our examples serve as a first consistency check in higher dimensions and lead to interesting results described above.

It is well known from quantum information theory that the entanglement negativity characterizes the upper bound on the distillable entanglement for mixed states. It is expected that our conjecture will lead to a deeper understanding of entanglement issues for diverse applications in higher dimensional conformal field theories from condensed matter physics to quantum gravity. It would be interesting to compute the holographic entanglement negativity for subsystems described by more general geometries other than the rectangular strip geometries considered by us. This would possibly lead to deeper insights into the nature of holographic quantum entanglement and its relation to issues of quantum gravity. We expect to return to these exciting issues in the near future.

7 Acknowledgment

Parul Jain would like to thank Prof. Mariano Cadoni for his guidance and the Department of Physics, Indian Institute of Technology Kanpur, India for their warm hospitality. Parul Jain’s work is financially supported by Università di Cagliari, Italy and INFN, Sezione di Cagliari, Italy.

References