Covariant Holographic Entanglement Negativity Conjecture for Adjacent Subsystems in $\mathrm{AdS_{3}/CFT_2}$

We propose a covariant holographic entanglement negativity conjecture for time dependent mixed states of adjacent intervals in $(1+1)$-dimensional conformal field theories dual to non-static bulk $\mathrm{AdS_3}$ configurations. Our conjecture applied to $(1+1)$-dimensional conformal field theories with a conserved charge dual to non-extremal and extremal rotating BTZ black holes exactly reproduces the corresponding replica technique results, in the large central charge limit. We also utilize our conjecture to obtain the time dependent holographic entanglement negativity for the mixed state in question for the $(1+1)$- dimensional CFT dual to a bulk Vaidya-$\mathrm{AdS_3}$ configuration.


I. INTRODUCTION
Quantum entanglement is one of the most intriguing aspects of quantum information theory which still eludes a complete understanding. Recent advances in this area have led to significant implications across diverse fields from condensed matter physics to quantum gravity. In this context entanglement entropy has emerged as a crucial measure to characterize the entanglement of bipartite quantum systems in pure states. This measure is defined as the von Neumann entropy for the reduced density matrix of the corresponding subsystem under consideration. Although it is straightforward to compute this quantity for systems with finite degrees of freedom, it is a complex and subtle issue for extended quantum many body systems. Despite this complication, a replica technique allows a systematic approach for the computation of this quantity in (1 + 1)-dimensional conformal field theories (CFT 1+1 ) [1,2].
It is well known in quantum information theory that the entanglement entropy is a valid measure for characterizing the entanglement of bipartite systems in pure states only. The issue of mixed state entanglement on the other hand is still an active area of research in the subject. For such mixed quantum states the entanglement entropy receives contributions from correlations which are not relevant for characterizing the entanglement of the bipartite system in question. In a classic communication [3], Vidal and Werner addressed this significant issue and proposed a computable measure termed entanglement * parul.jain@ca.infn.it † vinaymm@iitk.ac.in ‡ sayidphy@iitk.ac.in § sengupta@iitk.ac.in negativity which led to an upper bound on the distillable entanglement. Interestingly in [4][5][6], the authors computed the entanglement negativity for various mixed states in CFT 1+1 employing a variant of the replica technique mentioned earlier.
The replica technique developed in [4,5], was employed in [7] to investigate the entanglement negativity for time dependent mixed states of adjacent and disjoint intervals, following a global quench in a CFT 1+1 . Furthermore the time evolution of entanglement negativity following a local quench has been studied for two independently thermalized semiinfinite halves in a CFT 1+1 [8] and for harmonic chain out of equilibrium in [9]. The behavior of entanglement negativity following a local quench for the time dependent mixed states of symmetric and asymmetric adjacent and disjoint intervals in a CFT 1+1 has been investigated by utilizing the replica technique in [10]. Interestingly both for local and global quenches in a CFT 1+1 it was demonstrated in [7,10] that the universal parts of the entanglement negativity and mutual information show identical behavior for the time dependent mixed state of the adjacent intervals.
In the context of the AdS/CFT correspondence Ryu and Takayanagi (RT) [11,12] proposed an elegant holographic conjecture for the entanglement entropy of d-dimensional boundary CFTs (CFT d ) dual to bulk AdS d+1 configurations. The holographic entanglement entropy S γ in this instance could be described in terms of the area A γ of a co-dimension two bulk static minimal surface anchored on the subsystem γ under consideration as follows where G (d+1) N is the (d + 1)-dimensional Newton constant. Since its proposal the Ryu and Takayanagi conjecture has led to intensive research providing significant insights into the connections between spacetime geometry and entanglement [13][14][15][16][17][18][19][20][21].
The Ryu-Takayanagi [11,12] conjecture described above refers to the time independent entanglement in holographic CFTs which are dual to bulk static AdS configurations. For time dependent entanglement scenarios it is necessary to determine the precise definition of minimal surfaces for spacetime geometries with a Lorentzian signature. For such Lorentzian signature it is possible to contract a spacelike surface in the time direction to make its area arbitrarily small. This issue was resolved in a significant communication by Hubeny, Rangamani and Takayanagi (HRT) in which they proposed a covariant holographic conjecture for the entanglement entropy of CFTs dual to non-static bulk AdS gravitational configurations [22]. Their conjecture involves the light sheet construction arising from the covariant Bousso entropy bound [23][24][25] to describe the time dependent holographic entanglement entropy S At of a subsystem A t in terms of the area of co-dimension two bulk extremal surface Y ext At as follows ( This elegant covariant HRT conjecture has been extensively employed to investigate various time dependent entanglement issues for holographic CFTs [26][27][28][29][30][31]. As stated earlier the entanglement entropy fails to be a valid measure for characterizing mixed state entanglement in quantum information. Thus the holographic entanglement entropy conjectures of RT and HRT are applicable only for characterizing pure state entanglement in holographic CFTs. In the recent past two of the present authors (VM and GS) in the collaborations [32,33] proposed an elegant conjecture for the entanglement negativity of holographic CFTs (see also the discussions in [34] and for recent applications see [35]). A covariant entanglement negativity conjecture for time dependent mixed state entanglement in holographic CFTs was subsequently proposed in [36].
Note that the entanglement negativity conjecture in [32,33] refers to the mixed state entanglement between a single subsystem with the rest of the system in a holographic CFT. Motivated by the above construction very recently the present authors have proposed another distinct holographic entanglement negativity conjecture relevant for mixed states of adjacent subsystems in a holographic CFT [37,38]. Remarkably in the AdS 3 /CFT 2 context [37] this independent conjecture exactly reproduces the entanglement negativity of a holographic CFT 1+1 obtained through the replica technique, [4,5] in the large cen-tral charge limit [39].
In this article we advance a covariant holographic conjecture to describe the time dependent entanglement negativity for mixed states of adjacent intervals in holographic CFT 1+1 s dual to non-static bulk AdS 3 configurations. The time dependent holographic entanglement negativity in the AdS 3 /CFT 2 scenario described above involves a specific algebraic sum of the lengths of extremal curves anchored on the corresponding intervals. Interestingly, this reduces to the holographic mutual information between the adjacent intervals up to a numerical factor. We employ our holographic conjecture for the AdS 3 /CFT 2 scenario to compute the entanglement negativity of such mixed states in CFT 1+1 s with a conserved charge which are dual to bulk non-extremal and extremal rotating BTZ black holes. Quite remarkably, our results exactly match with the entanglement negativity of such holographic CFT 1+1 s obtained by us through the replica technique, in the large central charge limit. Interestingly, we observe that the covariant entanglement negativity for the holographic CFT 1+1 s dual to non-extremal rotating BTZ black holes decomposes into left and right moving sectors with distinct temperatures as described in [9]. Curiously, for the extremal rotating BTZ black holes, the holographic entanglement negativity characterized by a bulk Frolov-Thorne temperature [40], matches exactly with that obtained from the chiral half of the dual CFT 1+1 . Note that the above bulk configurations are stationary but not time dependent. As a consistency check for our covariant holographic negativity conjecture, we further compute the time dependent negativity for the mixed state described above in a CFT 1+1 dual to a bulk Vaidya-AdS 3 configuration. Very interestingly we observe numerically that the holographic negativity monotonically decreases with time clearly indicating the thermalization of the mixed state in question which corresponds to the black hole formation in the dual bulk AdS 3 geometry.
This article is organized as follows. In section II we very briefly recollect the essential elements of the HRT conjecture. Subsequently in section III we describe our covariant holographic entanglement negativity conjecture. In section IV we employ our conjecture to compute the covariant entanglement negativity for mixed states of adjacent intervals in holographic CFT 1+1 s dual to both non-extremal and extremal rotating BTZ black holes. In the subsequent section V we describe the computation for the entanglement negativity in the dual CFT 1+1 s for both the above cases, through the replica technique and compare these with the corresponding holographic results. In section VI we compute the time dependent holographic entanglement negativity for the mixed state in question, in a CFT 1+1 dual to a bulk Vaidya-AdS 3 configuration and analyses its time evolution.
In the final section VII we summarize our results and conclusions and describe interesting future open issues.

II. REVIEW OF HRT CONJECTURE
In this section we very briefly recollect the essential elements of the HRT conjecture [22] mentioned in the introduction. Their covariant holographic entanglement entropy conjecture crucially incorporates the light-sheet construction for the covariant Bousso entropy bound [23][24][25]. A light-sheet L S for a codimension two space like surface S in a space time manifold M is described by the congruence of null geodesics whose expansion is non-positive definite (θ ± ≤ 0, where θ ± are the future and the past null expansions respectively). The area of this surface S serves as a covariant bound on the entropy flux S LS (in Planck units) crossing through the light sheets as follows According to the HRT conjecture, the holographic entanglement entropy of a subsystem in a CFT d dual to a bulk AdS d+1 configuration, saturates the covariant Bousso bound described above. To this end the ddimensional boundary is bi partitioned into two space like regions A t and its complement A c t at a constant time t. The common (d − 2)-dimensional boundary shared by these two space like regions is denoted as ∂A t . The future and the past light sheets ∂L ± for this space like surface ∂A t are considered. These light sheets on the AdS boundary may then be extended into the bulk as L − and L + where they become the light sheets for a (d − 1)-dimensional space like surface Y At = L + ∩ L − anchored on the subsystem A t . The holographic proposal by HRT states that out of all such surfaces Y At , the entanglement entropy is determined by the surface which has minimal area (Y min At ). Furthermore, the authors also demonstrated that the surface (Y min At ) was actually the extremal surface (Y ext At ) anchored on the subsystem A t , with vanishing null expansions (θ ± = 0) leading to the saturation of the Bousso bound. The holographic entanglement entropy for the subsystem A t is therefore given as Having presented the essential elements of the HRT conjecture, in the next section we describe our covariant holographic conjecture for the entanglement negativity of mixed states described by adjacent subsystems in a boundary CFT 1+1 . Note that for the AdS 3 /CFT 2 scenario as mentioned in the Introduction the covariant holographic entanglement entropy involves the length of the extremal curve anchored on the corresponding interval.

III. COVARIANT HOLOGRAPHIC ENTANGLEMENT NEGATIVITY CONJECTURE FOR TWO ADJACENT SUBSYSTEMS
In this section we propose our covariant holographic conjecture for the time dependent entanglement negativity of the mixed state of adjacent subsystems in a holographic CFT 1+1 . To this end we begin with a brief description of our earlier holographic entanglement negativity conjecture for the corresponding time independent scenario in [37]. The holographic entanglement negativity between the adjacent intervals denoted as A 1 and A 2 was described through a specific algebraic sum of the lengths of bulk geodesics L γ anchored on the respective intervals γ For the time dependent scenario the covariant HRT conjecture [22] proposes that the entanglement entropy is described by the corresponding area of the co-dimension two bulk extremal surface anchored on the respective subsystem instead of the static minimal surface. As described in the previous section for the AdS 3 /CFT 2 scenario the HRT conjecture for the entanglement entropy involves length of the bulk extremal curve anchored on the corresponding interval. This motivates us to propose a holographic conjecture for the time dependent entanglement negativity for the mixed state of adjacent intervals in the AdS 3 /CFT 2 scenario as follows Here L ext are lengths of extremal curves in the bulk anchored on the respective subsystems on the boundary. It may be shown using the HRT conjecture that the above expression reduces to the holographic mutual information between the adjacent subsystems as follows where S γ is the entanglement entropy of a subsystem γ Eq. (4). It is interesting to note that the covariant holographic entanglement negativity for adjacent intervals is proportional to the holographic mutual information. Note that this holds only for the universal parts of these quantities which are dominant in the large central charge limit. Hence this does not indicate any contradiction with quantum information theory where they constitute distinct measures. Significantly for the same configuration it was shown by Tonni et. al. in [7] and by Ryu et. al. in [10], that the universal parts of these quantities had the same form in the context of global and local quenches in two dimensional conformal field theories.

IV. COVARIANT HOLOGRAPHIC NEGATIVITY FOR A CFT1+1 DUAL TO A ROTATING BTZ BLACK HOLE
In this section we employ our covariant holographic negativity conjecture described above to compute the entanglement negativity of mixed states of adjacent intervals in holographic CFT 1+1 s with a conserved charge, dual to bulk non-extremal and extremal rotating BTZ black holes.

A. Non-extremal BTZ
The non-extremal rotating BTZ (black string) metric with the AdS length scale set to unity (R = 1) is given as where the coordinate φ is non compact and r ± are the radii of the inner and outer horizons respectively. The mass M , angular momentum J, Hawking temperature T H , and the angular velocity Ω are related to the horizon radii r ± as follows The corresponding dual finite temperature CFT 1+1 with the bulk angular momentum J as the conserved charge, is defined on a twisted infinite cylinder 2 . The corresponding temperatures relevant to the left and the right moving modes in the dual CFT defined on the cylinder may now be expressed as follows The covariant holographic entanglement entropy S γ for a single spacelike interval γ at a constant time t = t 0 in the finite temperature holographic CFT 1+1 dual to the non-extremal rotating BTZ black hole is obtained from the HRT conjecture [22]. To this end it is necessary to perform the following coordinate transformations where u ± = φ ± t. These transformations map the BTZ metric Eq. (8) to the AdS 3 metric in the Poincaré coordinates as The corresponding length L γ of the geodesic anchored on the interval γ of length ∆φ = |φ 1 − φ 2 | in the holographic CFT 1+1 is then given as [22] L γ = log (∆φ) 2 ε i ε j , Here r ∞ and ε i (i = 1, 2) are the infra red cut-off for the bulk in the BTZ and the Poincaré coordinates respectively. This leads to the following expression for the geodesic length L γ in terms of the original BTZ coordinates as follows [22] where a is the UV cut-off for the boundary CFT 1+1 which is related to the bulk infra red cut-off as a = 1/r ∞ . We may now employ our covariant holographic negativity conjecture given in Eq. (6) for the mixed state 2 The fact that dual CFT 1+1 lives on a twisted cylinder can be observed from the conformal transformation given in eq. (27).
of adjacent intervals with lengths l 1 and l 2 in the holographic CFT 1+1 . This may be expressed as follows Note that the Brown-Henneaux formula c = 3R 2G 3

N
[41] has been used in the above expression. Interestingly we observe that the covariant holographic negativity for the mixed state in question decouples into E L and E R with left and right moving inverse temperatures β + and β − respectively [9]. We will have more to say about this issue in a later section.

B. Extremal BTZ
We now turn our attention to the covariant holographic negativity for the mixed state of adjacent intervals in holographic CFT 1+1 s with a conserved charge, dual to bulk extremal rotating BTZ black holes. The extremal rotating BTZ metric is given as In the extremal limit (r + = r − ), the mass M is equal to the angular momentum, J (M = J = 2r 2 0 ) and the corresponding Hawking temperature vanishes (T H = 0). As earlier, we first describe the computation for the length L γ of the bulk geodesic anchored on a interval γ of length ∆φ, in the rotating extremal BTZ geometry [22]. To this end is required to perform the following coordinate transformations which map the extremal BTZ metric Eq. (17) to the AdS 3 metric in the Poincaré coordinates (13) The geodesic length L γ anchored on the interval γ of length ∆φ may now be expressed as follows In the original BTZ coordinates the geodesics length in Eq. (19) reduces to the following It is now possible to employ our covariant holographic negativity conjecture for the mixed state of adjacent intervals with lengths l 1 and l 2 in the dual CFT 1+1 as follows where once again the Brown-Henneaux formula c = 3R 2G 3 N [41] has been used in the above expression and a is the UV cut off in the CFT 1+1 .
Note that the first term in the previous expression resembles the ground state entanglement negativity of the mixed state in question whereas the second term is the entanglement negativity at an effective temperature given by the well known Frolov-Throne temperature T FT = r0 π [40,42].

V. ENTANGLEMENT NEGATIVITY FOR A CFT1+1 DUAL TO A ROTATING BTZ BLACK HOLE
In this section we proceed to compute the entanglement negativity, through the replica technique, for the holographic CFT 1+1 dual to non extremal and extremal rotating BTZ black holes to establish the veracity of our conjecture. To this end we first describe the computation of the entanglement negativity for such mixed states in a generic CFT 1+1 given in [4,5]. The entanglement negativity for the mixed state of adjacent intervals with lengths l 1 and l 2 obtained through the replica technique is related to a three-point function of the twist fields as follows 3 3 Note that in [6], the authors study the entanglement negativity of a single interval with rest of the system in a finite temperature CFT 1+1 which requires a four point correlation of twist fields on an infinite cylinder. This is because of the complicated partial transpose over an infinite part of an infinite system at finite temperature. However this does not apply to the computation of the negativity for the mixed state of finite adjacent intervals which is still described by the three point function as given by eq. (22)  where n e stands for even parity of n and the limit n e → 1 is to be understood as an analytic continuation of even sequences of n to n e = 1 4 . The scaling dimensions for the twist fields in the above equation are given as follows [4,5] ∆ Tn e = c 12 n e − 1 n e , Note that the holographic CFT 1+1 s with a conserved charge, dual to both the non-extremal and the extremal rotating BTZ black holes live on a twisted infinite cylinder . These CFT 1+1 s are related to those defined on the complex plane through the appropriate conformal maps as described below. Hence the three point function in Eq. ( 22) for the entanglement negativity of the mixed state in question has to be evaluated on the corresponding twisted infinite cylinder. The transformation property of the three point in Eq. (22) under a conformal map (z → w) is given as follows where (z,z) are the coordinates on the plane and (w,w) are the coordinates on the twisted cylinder. The mixed state of the two adjacent intervals of lengths l 1 and l 2 may then be obtained by identifying the coordinates (w i ) on the cylinder as follows (25) Once the three-point function on the cylinder is obtained as described above, the corresponding entanglement negativity for the adjacent intervals case may then be computed by utilizing Eq. (22).

A. Non-extremal BTZ
We are now in a position to compute the entanglement negativity for the mixed state of adjacent intervals with lengths l 1 and l 2 in the finite temperature CFT 1+1 dual to a non-extremal rotating BTZ black hole. The partition function Z(β) for this dual finite temperature CFT 1+1 with the angular momentum J as the conserved charge are given as follows [22,42] Z(β) = Tr e −β(H−iΩE J) = Tr e −β+L0−β−L0 , (26) where ρ = e −β(H−iΩE J) is the corresponding density matrix, J is the angular momentum, Ω E = −iΩ is the Euclidean angular velocity and the Hamiltonian is H = L 0 +L 0 with L 0 andL 0 are the standard Virasoro zero modes. As stated earlier the non-extremal BTZ metric Eq. (8) is mapped to the Poincaré patch of AdS 3 by the coordinate transformations Eq. (12). Taking r ≫ r ± limit, one may determine the conformal map from the CFT 1+1 on the complex plane to that on the twisted infinite cylinder as follows The entanglement negativity of the mixed state in question may then be obtained through Eqs. (24), (27) and (22) which leads to the following expression where "constant" term is non universal and depends on the full operator content of the CFT 1+1 [4,5]. It was demonstrated in [37,39] that the non universal constant is sub leading in the large central charge limit and may be neglected. As earlier the entanglement negativity may be expressed as It is observed from the above expression that the universal part of the entanglement negativity for the CFT 1+1 decouples into E L and E R components with left and right moving inverse temperatures β + and β − respectively [9]. The separation of the entanglement negativity into these two parts correspond to the two mutually commuting chiral components of the relevant Hamiltonian H = L 0 +L 0 as described in [9]. Remarkably, the universal part of the entanglement negativity for the mixed state of adjacent intervals computed through the replica technique exactly matches with the corresponding results Eq. (16) obtained from our covariant holographic negativity conjecture.

B. Extremal BTZ
As described earlier the extremal BTZ metric (17) is mapped to the Poincaré patch of AdS 3 by the coordinate transformations Eq. (18). Note that as earlier the CFT 1+1 dual to the extremal BTZ black hole is also defined on a twisted infinite cylinder. The corresponding conformal map to the complex plane may be determined for the asymptotic limit (r → ∞) of the coordinate transformations Eq. (18) after a Wick rotation t → iτ as follows The entanglement negativity for the mixed state of adjacent intervals in the CFT 1+1 dual to the extremal BTZ black hole may then be obtained from Eq. (24), Eq. (30) and (22) which now leads to the following expression (31) It is important to note that the first term in the above expression is the entanglement negativity of the adjacent intervals for the CFT 1+1 in its ground state whereas the second term describes the entanglement negativity at an effective Frolov-Thorne temperature T F T [40,42]. As explained earlier the "constant" term is non universal and is sub leading in the large central charge limit [37,39]. Interestingly once again it is observed that the leading universal part of the entanglement negativity for the CFT 1+1 obtained through the replica technique exactly matches in the large central charge limit with the holographic result in Eq. (21) . Naturally this provides a strong consistency check for the universality of our conjecture in the AdS 3 /CF T 2 scenario.

VI. TIME DEPENDENT HOLOGRAPHIC ENTANGLEMENT NEGATIVITY
In the previous section we obtained the holographic negativity for the mixed state of adjacent intervals in CFT 1+1 s dual to bulk stationary AdS 3 geometry described by the rotating BTZ black holes. Note however that the full import of the covariant holographic negativity conjecture requires its application to time dependent mixed states in CFT 1+1 . To this end in this section we utilize our conjecture to compute the holographic entanglement negativity for time dependent mixed state configurations of adjacent intervals in a CFT 1+1 dual to a bulk Vaidya-AdS 3 space time. This bulk space time being one of the simplest examples of a time-dependent gravitational configuration in AdS 3 , describes the collapse process and subsequent black hole formation.
The Vaidya-AdS 3 metric in the Poincaré coordinates is given as [22,45] ds 2 = − r 2 − m(v) dv 2 + 2 dr dv + r 2 dx 2 , (32) where m(v) is a function of the (light cone) time v. If the mass function m(v) is a constant then this space time describes a non-rotating BTZ black hole.
The space like geodesic anchored on an interval of length l (x ∈ [−l/2, l/2]) in the CFT 1+1 dual to the bulk Vaidya-AdS 3 configuration is described by the functions r(x) and v(x) with the following boundary conditions Here, the UV cut-off r ∞ → ∞ which is inversely related to the lattice spacing as r ∞ = 1/ε. The length L of such a space like geodesic may be expressed as follows where thev andṙ represent the derivative of the functions v and r w.r.t the coordinate x. In order to compute the explicit form of the geodesic length L, we assume that the mass function m(v) is a slowly varying function of v andṁ(v) ≪ 1 in an adiabatic approximation as described in [22]. The length L of the space like geodesic described above may be written as [22] L = L reg + 2 log(2 r ∞ ), where the finite part of the length L reg of the space like geodesic is given as The covariant holographic entanglement negativity for the mixed state of adjacent intervals of lengths l 1 and l 2 may then be computed by utilizing our holographic conjecture Eq. (6). The finite part of the holographic entanglement negativity E f in may then be expressed as follows The finite part E f in in the above expression is obtained through the cut-off regularization i.e by subtracting the divergent part given below, from the full expression for the holographic entanglement negativity The characteristic behavior of the finite holographic entanglement negativity E f in as a function of v is depicted in fig. (1) with the choice of the mass function as m(v) = tanh v as described in [22,45]. Interestingly we observe that the absolute value of E f in decreases monotonically with v and saturates to a fixed value for large v describing the thermalization of the mixed state in question. Note that this corresponds to the black hole formation in the bulk AdS 3 geometry. Observe that the above plot is in contrast to that described in [22] for the holographic entanglement entropy involving the bulk Vaidya-AdS 3 geometry. The authors there demonstrated that the holographic entanglement entropy increases monotonically and saturates to the value of the thermal entropy for large v. It is a general expectation from quantum information theory that an entanglement measure has to be non-negative and that it is a monotonically decreasing function of the temperature [46]. Hence, entanglement negativity being an upper bound on the distillable entanglement for mixed quantum states is expected to decrease monotonically during the process of thermalization. On the other hand, the entanglement entropy receives contributions from both quantum and thermal correlations at finite temperatures and is dominated by the thermal correlations at high temperatures. As a result it increases monotonically as the mixed state thermalizes and saturates to the value of thermal entropy for large v.
Very interestingly, it has also been shown in the context of (1 + 1) dimensional quantum field theories at zero temperature, that the renormalized entanglement entropy (S ren A ) defined below, monotonically decreases along the renormalization group flow and is an example of an entropic c-function [47] S ren Here, l represents the length of an interval A. Such a well defined renormalized entanglement entropy is also expected to decrease monotonically under the renormalization group flow in higher dimensions [48,49] (See [50] for a recent review). Observe from fig.(1) that E f in is negative. The finite part of the entanglement negativity having negative values seems to be arising due to the cut-off regularization that we have utilized. It has been suggested in [51] that a well defined renormalized entanglement negativity may correspond to a generalized c-function which is non-negative and monotonically decreases with temperature from its UV (Low temperature) value to IR (High temperature) value. Hence, it follows that such an expression for the renormalized entanglement negativity decreases monotonically during the process of thermalization. Following [47,51], for the case of the adjacent intervals of equal length l 1 = l 2 = l, the renormalized entanglement negativity may be defined as Upon utilizing the length of the geodesics our conjec- ture given in Eq. (6) we may obtain the renormalized holographic entanglement negativity as The characteristic behavior of the renormalized holographic entanglement negativity (E ren ) as a function of v is depicted in fig. (2). Observe that as expected it is non-negative and a monotonically decreasing function of v. This clearly indicates that the renormalized holographic entanglement negativity decreases monotonically and saturates to a fixed value as the mixed state in question thermalizes.

VII. SUMMARY AND DISCUSSIONS
To summarize we have advanced a covariant holographic entanglement negativity conjecture for mixed states of adjacent intervals in (1+1)-dimensional conformal field theories dual to non-static bulk AdS 3 configurations. Our conjecture involves an algebraic sum of the lengths of bulk extremal curves anchored on the respective intervals. It is observed that the covariant holographic entanglement negativity reduces to the holographic mutual information between the corresponding intervals (in the large central charge limit of the CFT 1+1 ). Interestingly similar result for this configuration has been obtained in [7,10] in the context of global and local quenches in two dimensional conformal field theories.
To exemplify our conjecture and for a consistency check we have computed the entanglement negativity for the mixed state of adjacent intervals in CFT 1+1 s with a conserved charge, dual to the bulk stationary configurations described by non-extremal and extremal rotating BTZ black holes. For the finite temperature CFT 1+1 dual to the bulk non-extremal rotating BTZ black hole we demonstrated that the covariant holographic entanglement negativity decouples into two components involving corresponding left and right moving "temperatures". For the extremal rotating BTZ case on the other hand, the covariant entanglement negativity reduces to a sum of the negativity for the ground state dual to a bulk AdS vacuum and that of an effective "thermal" state characterized by a bulk Frolov-Thorne temperature.
To compare our holographic results we have computed the entanglement negativity through the replica technique for the dual CFT 1+1 s with a conserved charge. Remarkably, in both cases we are able to demonstrate that the covariant holographic entanglement negativity exactly reproduces the universal part of the corresponding replica technique results in the large central charge limit of the CFT 1+1 .
Furthermore to illustrate the time dependent aspect of our covariant holographic negativity conjecture we consider mixed states of adjacent intervals in a CFT 1+1 dual to a bulk Vaidya-AdS 3 geometry. Very interestingly we are able to show from our conjecture that the renormalized holographic entanglement negativity monotonically decreases with time and saturates to a small fixed value indicating the thermalization of the mixed state in question. As is well known this corresponds to the black hole forma-tion in the bulk AdS 3 geometry and is completely consistent with quantum information theory expectations for this process [46]. Naturally, these examples provide strong consistency checks for our proposed conjecture. The above results obtained utilizing our conjecture in the AdS 3 /CFT 2 scenario strongly motivate us to propose the generalization of our conjecture to higher dimensions in the spirit of [38]. Following [22], this leads us to generalize our covariant holographic entanglement negativity conjecture for the mixed state of adjacent subsystems in CFT d s dual the non-static bulk AdS d+1 configurations in terms of the areas of the extremal surfaces instead of the static minimal surfaces. This is expressed as follows where Y ext γ denotes the bulk extremal surface anchored on the corresponding subsystem γ. However, it would require us to put our conjecture through explicit checks for specific higher dimensional examples and provide a plausible proof. We leave these significant open issues for future investigations.
Our covariant holographic entanglement negativity conjecture provides an ingenious prescription to determine the entanglement negativity of time dependent mixed states in generic holographic CFTs. Naturally, this will have significant implications for time dependent entanglement issues such as entanglement evolution in quantum quenches and thermalization, quantum phase transitions and topological order in condensed matter physics. Our conjecture also promises significant insights into black hole formation and collapse scenarios, information loss paradox, unitarity restoration and the related firewall problem in the AdS 3 /CFT 2 context. We hope to address these fascinating open issues in the near future.

VIII. 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.