The entanglement negativity \( \mathcal{E} \) (A : B) is a useful measure of quantum entanglement in bipartite mixed states. In random tensor networks (RTNs), which are related to fixed-area states, it was found in ref. [1] that the dominant saddles computing the even Rényi negativity \( {\mathcal{E}}^{(2k)} \) generically break the ℤ2k replica symmetry. This calls into question previous calculations of holographic negativity using 2D CFT techniques that assumed ℤ2k replica symmetry and proposed that the negativity was related to the entanglement wedge cross section. In this paper, we resolve this issue by showing that in general holographic states, the saddles computing \( {\mathcal{E}}^{(2k)} \) indeed break the ℤ2k replica symmetry.
Our argument involves an identity relating \( {\mathcal{E}}^{(2k)} \) to the k-th Rényi entropy on subregion AB∗ in the doubled state \( {\left.|{\rho}_{AB}\right\rangle}_{A{A}^{\ast }{BB}^{\ast }} \) , from which we see that the ℤ2k replica symmetry is broken down to ℤk. For k < 1, which includes the case of \( \mathcal{E} \) (A : B) at k = 1/2, we use a modified cosmic brane proposal to derive a new holographic prescription for \( {\mathcal{E}}^{(2k)} \) and show that it is given by a new saddle with multiple cosmic branes anchored to subregions A and B in the original state. Using our prescription, we reproduce known results for the PSSY model and show that our saddle dominates over previously proposed CFT calculations near k = 1. Moreover, we argue that the ℤ2k symmetric configurations previously proposed are not gravitational saddles, unlike our proposal. Finally, we contrast holographic calculations with those arising from RTNs with non-maximally entangled links, demonstrating that the qualitative form of backreaction in such RTNs is different from that in gravity.
