Covariant holographic entanglement negativity for disjoint intervals in $AdS_3/CFT_2$

We advance a construction for the covariant holographic entanglement negativity of time dependent mixed states of disjoint intervals in $(1+1)$ dimensional conformal field theories ($CFT_{1+1}$) dual to bulk non static $AdS_3$ geometries. Application of our proposal to such mixed states in a $CFT_{1+1}$ dual to bulk non extremal and extremal rotating BTZ black holes exactly reproduces the replica technique results in the large central charge limit. We also investigate the time dependent holographic entanglement negativity for such mixed states in a $CFT_{1+1}$ dual to a bulk Vaidya-$AdS_3$ geometry in the context of their thermalization involving bulk black hole formation.


Introduction
Recently quantum entanglement has emerged as one of the most active research areas garnering interest from a diverse range of fields extending from condensed matter physics to quantum gravity. For bipartite pure states the entanglement may be characterized by the entanglement entropy measure, defined as the von Neumann entropy of the reduced density matrix for the corresponding subsystem. This is difficult to compute for extended quantum many body systems with infinite degrees of freedom although a formal definition may be characterized through a replica technique. For (1 + 1) dimensional conformal field theories however the entanglement entropy may be explicitly computed through the replica technique as described in [1,2].
It is well known from quantum information theory that the entanglement entropy fails to characterize mixed state entanglement as it receives contributions from correlations irrelevant to the entanglement of the mixed state in question. This crucial issue was addressed in a significant communication by Vidal and Werner through the introduction of a computable measure termed entanglement negativity (logarithmic negativity) characterizing the upper bound on the distillable entanglement for mixed states [3]. 1 This measure was defined as the logarithm of the trace norm of the partially transposed reduced density matrix of a bipartite system with respect to one of the subsystems. In [4] it was observed that this measure although not convex, was an entanglement monotone under local operations and classical communication (LOCC).
A variant of this replica technique was later developed to compute the entanglement negativity for various mixed states in CF T 1+1 s [5][6][7]. Subsequently this technique was extended to compute the entanglement negativity following a global quench for time dependent mixed states of disjoint and adjacent intervals in a CF T 1+1 [8]. The time evolution of the entanglement negativity for certain mixed states in a CF T 1+1 following a local quench could then be investigated in [9][10][11].
In a significant communication Ryu and Takayanagi [12,13] (RT) advanced a holographic conjecture for the entanglement entropy of a subsystem in a CF T d dual to a bulk AdS d+1 geometry in the AdS/CF T scenario. The entanglement entropy was found to be proportional to the area of a co dimension two bulk static minimal surface anchored on the subsystem. The RT conjecture inspired intense activity in this area leading to several interesting insights [14][15][16] and references therein. However the RT conjecture described above was valid only for a time independent scenario. For time dependent configurations it was required to formulate the precise characterization of minimal surfaces in the context of a Lorentzian signature space time.
In [17] Hubeny, Rangamani and Takayanagi (HRT) addressed this crucial issue and proposed a covariant holographic conjecture for the entanglement entropy in a CF T d dual to a non static bulk AdS d+1 geometry. Their proposal involved the light sheet construction leading to the covariant Bousso entropy bound [18][19][20]. In this time dependent scenario the holographic entanglement entropy of a subsystem in a CF T d could be described in terms of the area of a co dimension two bulk extremal surface anchored on the subsystem. The HRT conjecture was subsequently utilized to obtain the entanglement entropy for various time dependent configurations in holographic CF T s [21][22][23][24][25][26].
The developments described above leads to the significant issue of a holographic characterization for the entanglement negativity of mixed state configurations in a dual CF T d . In [27,28] two of the present authors (VM and GS) advanced a holographic entanglement negativity conjecture for mixed state configurations in holographic CF T s. Its covariant extension for the time dependent mixed state entanglement was subsequently proposed in [29]. Following this it was possible to obtain the holographic entanglement negativity for mixed state configurations of adjacent subsystems in a dual CF T [30,31]and its covariant generalization in [32].
Very recently in [33] we have obtained the holographic entanglement negativity for the interesting mixed state configuration of disjoint subsystems in proximity in a holographic CF T 1+1 . In this case the replica technique requires the computation of a four point twist correlator in the CF T 1+1 leading to the entanglement negativity which involves a non universal function of the cross ratio. Using a monodromy technique it was possible to extract a universal part for the four point twist correlator above in the large central charge limit. The resulting large c expression for the entanglement negativity exhibited universal features consistent with known results described in [30]. In [34], the entanglement entropy for the configuration of two disjoint intervals was shown to exhibit a phase transition depending on the value of the four point cross ratio x. The transition occurred between its values in the s-channel (x → 0) and the t-channel (x → 1) at x = 1 2 . In the dual bulk AdS 3 space time, this involved distinct geodesic combinations anchored on appropriate intervals. A similar phase transition was reported for the entanglement negativity of the mixed state of two disjoint intervals in [35].
In this article we advance a covariant holographic entanglement negativity construction for mixed state configurations of disjoint intervals in a CF T 1+1 through a large central charge analysis as described above for the case of a static bulk configuration. Our construction provides a characterization for the time dependent entanglement for the mixed states in question in a holographic CF T 1+1 dual to non static bulk AdS 3 geometry. The holographic construction involves a specific algebraic sum of the lengths of bulk extremal curves anchored on appropriate subsystems relevant to the mixed state under consideration which reduces to an algebraic sum of the holographic mutual informations between specific subsystems. Our proposal is then utilized to obtain the holographic entanglement negativity for such mixed state configurations in a CF T 1+1 with a conserved charge, dual to bulk non extremal and extremal rotating BTZ black holes. As a consistency check for our construction we subsequently compute the entanglement negativity for such mixed states in these specific holographic CF T 1+1 s through a replica technique in the large central charge limit. Quite significantly the results obtained from our holographic construction match exactly with the corresponding replica technique results obtained in the large central charge limit. Interestingly in the limit of adjacent intervals our results reproduce those described in [32] and constitutes an additional substantiation of our construction. Note that the examples described above refers to CF T 1+1 s dual to bulk AdS 3 geometries. In order to elucidate the full implications of our holographic construction we subsequently obtain the time dependent holographic entanglement negativity for the mixed state under consideration in a CF T 1+1 dual to a time dependent bulk Vaidya-AdS 3 geometry. Very significantly for this example we demonstrate that the holographic entanglement negativity decreases monotonically with time illustrating the thermalization of the mixed state which corresponds to the formation of a black hole in the bulk.
This article is organized as follows. In section 2 we briefly review the HRT conjecture for the entanglement entropy. In section 3 we describe our covariant holographic entanglement negativity construction. Subsequently in section 4 we utilize our proposal to obtain the holographic entanglement negativity for mixed state configurations of disjoint intervals in CF T 1+1 s dual to bulk non extremal and extremal rotating BTZ black holes. In section 5, we obtain the entanglement negativity for the mixed states described above in the specific dual CF T 1+1 s through a replica technique in the large central charge limit and compare these with the results obtained using our holographic construction. Following this in section 6, we apply our proposal to obtain the holographic entanglement negativity of two disjoint intervals in a CF T 1+1 dual to a time dependent bulk Vaidya-AdS 3 configuration. Finally in section 7 we present a summary of our results and conclusions.

Review of the HRT conjecture
We begin by briefly reviewing the HRT conjecture as described in [17]. Their elegant prescription for the covariant holographic entanglement entropy involves the light sheet construction proposed by Bousso [18][19][20]. In this construction the congruence of null geodesics with non positive definite expansion specifies a light sheet L S for a space like surface S of co dimension two in a space time manifold M. A covariant upper bound (Bousso entropy bound) for the entropy flux S L S (in Planck units) passing through the light sheets of the space like surface S above is described by its area as follows The HRT conjecture states that the equality sign in the above relation holds for the holographic entanglement entropy of a subsystem in a CF T d dual to a bulk AdS d+1 configuration. In this context the d dimensional boundary of AdS d+1 is divided into two space like regions A t and its complement A c t at a fixed time t. The resulting (d − 2) dimensional space like surface serving as the common boundary to these two space like regions is denoted by ∂A t . The future and the past light sheets ∂L ± for this surface, when extended into the bulk as L ± , serve as the light sheets of a (d − 1) dimensional bulk space like surface Y At = L + ∩ L − anchored on the subsystem A t . It was proposed that amongst all such surfaces Y At , the one with the minimal area, denoted by Y min At , determines the holographic entanglement entropy of the subsystem A t . It was further shown that this minimal surface Y min At is the extremal surface Y ext At anchored on the subsystem A t . Interestingly the surface Y ext At has vanishing null expansions, which explains the saturation of the covariant Bousso bound. The holographic entanglement entropy for the subsystem A t is hence given by In this regard we note that in the context of the AdS 3 /CF T 2 scenario, the covariant holographic entanglement entropy will involve the lengths of space like bulk extremal curves (geodesics) anchored on the corresponding spatial intervals. This concludes our brief review of the HRT construction.

Covariant holographic entanglement negativity for two disjoint subsystems
In this section we propose our covariant holographic entanglement negativity prescription for time dependent mixed state configurations of disjoint intervals in a CF T 1+1 in the boundary, dual to a non static bulk AdS 3 geometry. In this context we first briefly outline our previous holographic construction for the entanglement negativity of such mixed state configurations in the corresponding time independent case [33]. The entanglement negativity for the mixed state of disjoint intervals A 1 ∈ [u 1 , v 1 ] (of length l 1 ) and A 2 ∈ [u 2 , v 2 ] (of length l 2 ), separated by the interval A S ∈ [v 1 , u 2 ] (of length l s ) in the dual CF T 1+1 as illustrated in figure 1, may be obtained through a replica technique involving a specific four point twist correlator as follows (3) Here we have identified The limit n e → 1 is taken through an analytic continuation of even sequences {n e } to n e = 1.
The four point twist correlator in eq. (3) is in general non universal and depends on the full operator content of the underlying theory as described in [6]. However, for two disjoint intervals in proximity (described by the condition 1/2 < x < 1), in the large central charge limit, the following universal form may be obtained through the monodromy technique [34][35][36] Here the four point cross ratio x is given by ( The two point twist correlator in a holographic CF T 1+1 is given as Using the AdS 3 /CF T 2 dictionary this two point twist correlator (in the geodesic approximation) may be described in terms of the length L ij of the space like geodesic in the bulk, anchored on the corresponding interval in the boundary as follows [13] T with R being the AdS 3 length scale. Utilizing eqs. (6) and (7), it is now possible to express the four point twist correlator given in eq. (4) as follows From the expression for the four point twist correlator in eq. (8) and using eq. (3) the holographic entanglement negativity for the mixed state configuration of the two disjoint intervals in proximity may be expressed as Here the Brown-Henneaux formula c = 3R
According to the HRT conjecture the computation of holographic entanglement entropy in the time dependent scenario involves the area of the corresponding co dimension two bulk extremal surface anchored on the respective subsystem in the boundary. In the context of the AdS 3 /CF T 2 scenario these are extremal curves anchored on the corresponding intervals. This motivates us to propose the following covariant construction for the time dependent holographic entanglement negativity of the mixed state configuration of two disjoint intervals in proximity in the AdS 3 /CF T 2 framework as where L ext γ denotes the length of the bulk space like extremal curve anchored on the subsystem (γ) in the dual CF T 1+1 . Note that here A t i denotes the subsystem A i at a fixed time t as described earlier in section 2. The HRT conjecture described in eq. (2) may now be utilized to arrive at the following The covariant holographic entanglement negativity described in eq. (11) may be further expressed in terms of a specific sum of the holographic mutual informations between appropriate combinations of the subsystems as follows 2 Here the holographic mutual information between the subsystems A t i and A t j is given by Interestingly in the limit A t s → ∅, we recover the exact expression as reported in [32] for the the mixed state holographic entanglement negativity of adjacent intervals in terms of the holographic mutual information between the subsystems A t 1 and A t 2 .
4 Covariant holographic entanglement negativity in CF T 1+1 dual to rotating BTZ black holes In this section we utilize our covariant holographic construction as described in eq. (10) above, to compute the time dependent entanglement negativity for mixed states of two disjoint intervals in proximity in a CF T 1+1 with a conserved charge, dual to bulk non extremal and extremal rotating BTZ black holes.

Non extremal BTZ black hole
We first focus on the CF T 1+1 with a conserved charge dual to the non extremal rotating BTZ (black string) whose metric (with the AdS 3 radius R set to unity) is given as where the coordinate φ is non compact and r ± denote the radii of the inner and the outer horizons respectively. The mass M , angular momentum J, Hawking temperature T H , and the angular velocity Ω may be expressed in terms of the horizon radii r ± as follows The finite temperature dual CF T 1+1 with the bulk angular momentum J as the conserved charge may be defined on a twisted infinite cylinder. 3 The temperatures relevant to the left and the right moving modes respectively in the dual CF T are given as To obtain the lengths of the extremal curves (which are space like geodesics) in this bulk geometry we map the BTZ metric in eq. (13) to the Poincaré patch of the AdS 3 space time as follows where u ± = φ ± t. The resulting AdS 3 metric is then given by The length of the space like geodesic in this bulk geometry, which is anchored on an interval γ of length ∆φ = |φ 1 − φ 2 | in the dual CF T 1+1 , may now be obtained as follows [17] Here r ∞ and ε i (i, j = 1, 2) denote the infra red cut offs for the bulk in the BTZ and the Poincaré coordinates respectively. Using the above expressions in eq. (18) the geodesic length L γ may now be expressed in terms of the original BTZ coordinates as follows [17] L γ = ln Here a is the UV cut off of the CF T 1+1 in the boundary which is related to the bulk infra red cut off r ∞ through the AdS/CF T dictionary by a = 1/r ∞ . The covariant holographic entanglement negativity for the mixed state configuration of disjoint intervals in proximity in the CF T 1+1 with a conserved charge, dual to the non extremal BTZ black hole in the bulk, may now be obtained by utilizing our covariant holographic negativity construction described by eq. (10) as follows E = c 8 ln   sinh π(l 1 +ls) β + sinh π(l 2 +ls) β + sinh πls β + sinh π(l 1 +l 2 +ls) Here l 1 and l 2 denote the respective lengths of the disjoint intervals and their separation is given by l s and L/R denotes the left and the right moving sector in the dual CF T 1+1 . Note that the covariant holographic entanglement negativity in this case decouples into E L and E R with the left and right moving inverse temperatures β + and β − respectively [10]. It is interesting to note that the above expression for entanglement negativity for the mixed state configuration of disjoint intervals is independent of the UV cut off a. When the intervals in question are adjacent (obtained through the limit l s → a), the above expression in eq. (20) exactly reproduces the corresponding entanglement negativity result in [32].

Extremal BTZ black hole
Having computed the holographic entanglement negativity for the mixed state of disjoint intervals in a CF T 1+1 dual to a bulk non extremal rotating BTZ black hole, we now turn our attention to the corresponding case in a CF T 1+1 dual to an an extremal rotating BTZ black hole. The metric for the dual bulk extremal black hole in the BTZ coordinates is given by In this extremal limit described by r + = r − = r 0 , the Hawking temperature vanishes (T H = 0), whereas the mass and the angular momentum coincide M = J = 2r 2 0 . To compute the bulk space like geodesic lengths L γ as earlier, we first consider the coordinate transformation mapping the extremal BTZ metric in eq. (21) to the AdS 3 metric in the Poincaré coordinates given in eq. (17) as follows The length L γ of the space like bulk geodesic anchored on the interval γ of length ∆φ may then be obtained as [17] L where i, j = {1, 2}. Finally, the above expression for the space like bulk geodesic length L γ in eq. (23) may be expressed in the original BTZ coordinates as follows We now utilize our covariant construction described in eq. (10) to obtain the holographic entanglement negativity for the mixed state configuration of disjoint intervals in proximity in the CF T 1+1 under consideration as follows Once again we note that this result is independent of the UV cut off. Interestingly the holographic entanglement negativity in the above expression decouples into two independent parts with distinct significances. The first term is exactly half of the corresponding holographic entanglement negativity for the zero temperature mixed state configuration of two disjoint intervals in proximity described in [33]. The second term on the other hand resembles the finite temperature entanglement negativity of the mixed state configuration in question, at the Frolov-Throne temperature T F T = r 0 π [38,39]. As earlier in the adjacent limit (l s → a), our result in eq. (25) exactly reproduces the corresponding holographic entanglement negativity of the mixed state configuration of adjacent intervals described in [32].

Entanglement negativity for disjoint intervals in CF T 1+1 dual to rotating BTZ black holes
In this section we compute the entanglement negativity for the mixed state configurations of disjoint intervals in proximity in CF T 1+1 s dual to non extremal and extremal rotating BTZ black holes, through a replica technique and compare with the corresponding holographic results obtained in the previous section. This serves as a strong consistency check for our holographic construction. For this purpose we briefly recapitulate the essential elements of the computation of entanglement negativity for such mixed states in a generic CF T 1+1 described in [5,6,33].
We begin by noting that for the case of a CF T 1+1 on the complex plane, a universal form for the four point twist correlator in the large central charge limit has been obtained in [36], as described earlier in eq. (4). On the other hand CF T 1+1 s with a conserved charge dual to non extremal and the extremal rotating BTZ black holes must be defined on twisted infinite cylinders (see footnote 3). Hence the four point twist correlator in eq. (4) for such CF T 1+1 s are computed on such twisted cylinders. The corresponding conformal maps from the complex plane to these twisted cylinders are described in the following subsections. The transformation property of the four point twist correlator in eq. (4) under a conformal map z → w is given as follows where ∆ i are the scaling dimensions of the twist fields at the locations z = z i . Here z and w are the coordinates on the plane and the twisted cylinder respectively.
The entanglement negativity for the mixed state of the two disjoint intervals described above may then be computed by utilizing eqs. (3), (4) and (26) by identifying the coordinates (w i ) on the cylinder as w 1 ≡ u 1 , w 2 ≡ v 1 , w 3 ≡ u 2 , w 4 ≡ v 2 , as described below.

Non extremal BTZ black hole
We now proceed to compute the entanglement negativity for the mixed state configuration of disjoint intervals in proximity in the finite temperature CF T 1+1 dual to a non extremal rotating BTZ black hole. To this end we consider the partition function for this CF T , which is described as follows [17,39] Here ρ = exp [−β (H − iΩ E J)] is the appropriate density matrix, and the angular momentum which is a conserved charge is denoted by J. Ω E = −iΩ is the Euclidean angular velocity and the Hamiltonian is given by H = L 0 +L 0 where L 0 andL 0 are the standard Virasoro zero modes. As described earlier in subsection 4.1, the non extremal BTZ metric given in eq. (13) is mapped to the Poincaré patch of AdS 3 by the coordinate transformations described in eq. (16). In the limit r ≫ r ± , the conformal map from the CF T 1+1 on the complex plane to that on the twisted infinite cylinder reduces to Utilizing eqs. (3), (4), (26) and (28), the entanglement negativity of the mixed state in question in the large central charge limit may then be obtained as follows Note that the universal part of the entanglement negativity for the CF T 1+1 decouples into E L and E R components depending only on the left and right moving inverse temperatures β + and β − respectively [10] (see also the discussion after eq. (20)). This decoupling corresponds to the two mutually commuting chiral components of the Hamiltonian H = L 0 +L 0 as described in [10]. Significantly, the entanglement negativity for the mixed state configuration of disjoint intervals obtained in the large central charge limit exactly matches with the corresponding result in eq. (20) obtained from our covariant holographic entanglement negativity construction.

Extremal BTZ black hole
As stated earlier in subsection 4.2, the extremal BTZ metric given in eq. (21) is mapped to the Poincaré patch of AdS 3 by the coordinate transformations described in eq. (22). In the asymptotic limit (r → ∞), the relevant conformal map from the complex plane to the twisted infinite cylinder in this case may be obtained from the coordinate transformations described in eq. (22) after a Wick rotation t → iτ as follows Utilizing eqs. (3), (4), (26) and (30), the entanglement negativity for the mixed state configuration of disjoint intervals in proximity in the large central charge limit in the CF T 1+1 dual to an extremal BTZ black hole may then be determined as follows Significantly the first term in the above expression indicates the entanglement negativity of the disjoint intervals in proximity for the CF T 1+1 in its ground state while the second term describes the entanglement negativity at an effective Frolov-Thorne temperature T F T [38,39] (see the discussion after eq. (25)). Remarkably the entanglement negativity for the CF T 1+1 obtained through the replica technique in the large central charge limit matches exactly with the holographic result described in eq. (25). Once again this constitutes a robust consistency check for our holographic construction.

Time dependent holographic entanglement negativity
In the earlier sections we have described the application of our covariant holographic entanglement negativity construction to time independent mixed state configuration of disjoint intervals in proximity in CF T 1+1 s dual to stationary bulk AdS 3 configurations and compared our results with those obtained through a replica technique. However note that our covariant holographic construction is also valid for mixed states with explicit time dependence in CF T 1+1 s. In this section we address this significant issue of time dependent mixed state entanglement through our covariant holographic entanglement negativity construction described in section 3. In this context we obtain the holographic entanglement negativity for the time dependent mixed state configuration of disjoint intervals in proximity in a CF T 1+1 dual to a bulk Vaidya-AdS 3 configuration. This bulk AdS 3 geometry characterizes one of the simplest time dependent gravitational configurations and describes the collapse process and subsequent black hole formation. The Vaidya-AdS 3 metric may be described in the Poincaré coordinates as [17,40] Here m(v) denotes the mass function for the light cone time v. For a constant m(v), the above metric describes a non rotating BTZ black hole. In this scenario, the space like geodesic in the bulk Vaidya-AdS 3 , anchored on the interval x ∈ [−l/2, l/2] (of length l) in the dual CF T 1+1 , may be characterized by the functions r(x) and v(x) of the boundary spatial coordinate x with the boundary conditions given as Here the UV cut off r ∞ = 1/ε, where ε is the lattice spacing. The length of the space like geodesic described above may be given as wherev andṙ denote the derivatives of the functions v and r with respect to the coordinate x respectively.
To extract an explicit form of the geodesic length L from the above expression, it is required to employ the adiabatic approximation as outlined in [17] wherein the mass function m(v) is assumed to be a slowly varying function of v andṁ(v) ≡ dm dv / dx dv ≪ 1. The length L of the bulk space like geodesic may then be computed as [17] L = L reg + 2 ln (2r ∞ ) .
Here the regularized part L reg of the length of the space like geodesic as mentioned in the above expression is given as We may now use the expression for L in eq. (34) to compute the covariant holographic entanglement negativity for the mixed state of disjoint intervals in proximity by utilizing our holographic conjecture as described in eq. (10) as follows Interestingly, unlike the case for adjacent intervals described in [32], for the case of disjoint intervals, the entanglement negativity has no divergent part.
In figure 2, we plot the entanglement negativity as a function of v for different sizes of the intervals. For this we have chosen the mass function as m(v) = tanh v as described in [17,40]. In all the cases, the entanglement negativity decreases monotonically with v and eventually saturates for large v, which characterizes the thermalization of the mixed state under consideration. This thermalization corresponds to the black hole formation in the bulk. This result is completely consistent with quantum information theory expectations [41]. In quantum information theory an entanglement measure is expected to be non-negative and a monotonically decreasing function of the temperature [41]. The behavior of the entanglement negativity in figure 2 is consistent with the above expectations and the fact that it characterizes the upper bound on the distillable entanglement for mixed states. This is in contrast to the corresponding behavior of the holographic entanglement entropy involving the bulk Vaidya-AdS 3 geometry, where it increases monotonically and saturates to the value of the thermal entropy for large v [17]. At finite temperatures, the entanglement entropy receives contributions from both quantum and thermal correlations, and is dominated by the thermal correlations at high temperatures. Hence it increases monotonically as the mixed state thermalizes and saturates to the value of the thermal entropy for large v.

Summary and conclusions
To summarize we have established a covariant holographic entanglement negativity construction for time dependent mixed state configurations of disjoint subsystems in proximity in (1 + 1) dimensional conformal field theories dual to non static bulk AdS 3 geometries. To this end a large central charge analysis for the corresponding replica technique results in the dual CF T 1+1 has been utilized. Our construction involves a specific algebraic sum of the lengths of bulk extremal curves anchored on appropriate combinations of the intervals. This may also be expressed in terms of the holographic mutual informations between specific combinations of the intervals involved.
In this context we have obtained the holographic entanglement negativity for the mixed state configurations of disjoint intervals in proximity in CF T 1+1 s dual to specific bulk geometries. These include CF T 1+1 s with a conserved charge, dual to stationary bulk AdS 3 configurations described by non extremal and extremal rotating BTZ black holes. Our results for these cases match exactly with the corresponding replica technique results in the large central charge limit. These serve as strong consistency checks for our construction. Interestingly the covariant holographic entanglement negativity decouples into two parts corresponding to the left and right moving temperatures in the finite temperature CF T 1+1 dual to the bulk non extremal rotating BTZ black hole. For the extremal rotating BTZ case on the other hand, it decouples into the entanglement negativity for the ground state in a CF T 1+1 dual to a bulk pure AdS 3 geometry and that for a thermal state described by a bulk Frolov-Thorne temperature.
Furthermore we have utilized our construction to investigate the time dependent mixed state configuration of disjoint intervals in proximity in a CF T 1+1 dual to a bulk Vaidya-AdS 3 geometry. Remarkably we have been able to demonstrate the time dependent aspect of this configuration where the holographic entanglement negativity monotonically decreases with time leading to its eventual saturation to a small fixed value. This characterizes the thermalization of the mixed state in the CF T 1+1 under consideration, and corresponds to the formation of a bulk black hole. We emphasize that our covariant holographic entanglement negativity conjecture furnishes an elegant method to compute the holographic entanglement negativity of time dependent mixed state configurations in dual CF T 1+1 s. However although substantiated with non trivial examples a bulk proof for our construction along the lines of [42] is an outstanding issue. Our holographic construction also suggests a higher dimensional extension to a generic AdS d+1 /CF T d scenario involving co dimension two bulk extremal surfaces anchored on appropriate subsystems. Naturally such an extension would also require a bulk proof along the lines of [43].
Clearly our holographic construction proposed here will have significant impact for the investigation of time dependent entanglement issues such as time evolution of entanglement in quantum quenches and thermalization, black hole formation and collapse scenarios, information loss paradox, unitarity restoration and the related firewall problem in the context of AdS 3 /CF T 2 holography. These constitute interesting open issues for future investigations.