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arXiv:1503.07526 · Physical Review A

Degradation of entanglement between two accelerated parties: Bell states under the Unruh effect

Benedikt Richter, Yasser Omar

Published Aug 14, 2015• 59 citations
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Abstract

We study the entanglement of families of Unruh modes in the Bell states $|{\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\rangle}=1/\sqrt{2}(|00\ensuremath{\rangle}\ifmmode\pm\else\textpm\fi{}|11\ensuremath{\rangle})$ and $|{\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\rangle}=1/\sqrt{2}(|01\ensuremath{\rangle}\ifmmode\pm\else\textpm\fi{}|10\ensuremath{\rangle})$ shared by two accelerated observers and find fundamental differences in the robustness of entanglement against acceleration for these states. States ${\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}$ are entangled for all finite accelerations, whereas, due to the Unruh effect, states ${\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}$ lose their entanglement for finite accelerations. This is true for Bell states of two bosonic modes, as well as for Bell states of a bosonic and a fermionic mode. Furthermore, there are also differences in the degradation of entanglement for Bell states of fermionic modes. We reveal the origin of these distinct characteristics of entanglement degradation and discuss the role that is played by particle statistics. Our studies suggest that the behavior of entanglement in accelerated frames strongly depends on the occupation patterns of the constituent states, whose superposition constitutes the entangled state, where especially states ${\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}$ and ${\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}$ exhibit distinct characteristics regarding entanglement degradation. Finally, we point out possible implications of hovering over a black hole for these states.

DOI
10.1103/physreva.92.022334

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We study the entanglement of families of Unruh modes in the Bell states ∣\ensuremathΦ\ifmmode±\else\textpm\fi\ensuremath⟩=1/2(∣00\ensuremath⟩\ifmmode±\else\textpm\fi∣11\ensuremath⟩)|{\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\rangle}=1/\sqrt{2}(|00\ensuremath{\rangle}\ifmmode\pm\else\textpm\fi{}|11\ensuremath{\rangle})∣\ensuremathΦ\ifmmode±\else\textpm\fi\ensuremath⟩=1/2​(∣00\ensuremath⟩\ifmmode±\else\textpm\fi∣11\ensuremath⟩) and ∣\ensuremathΨ\ifmmode±\else\textpm\fi\ensuremath⟩=1/2(∣01\ensuremath⟩\ifmmode±\else\textpm\fi∣10\ensuremath⟩)|{\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremath{\rangle}=1/\sqrt{2}(|01\ensuremath{\rangle}\ifmmode\pm\else\textpm\fi{}|10\ensuremath{\rangle})∣\ensuremathΨ\ifmmode±\else\textpm\fi\ensuremath⟩=1/2​(∣01\ensuremath⟩\ifmmode±\else\textpm\fi∣10\ensuremath⟩) shared by two accelerated observers and find fundamental differences in the robustness of entanglement against acceleration for these states. States \ensuremathΨ\ifmmode±\else\textpm\fi{\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathΨ\ifmmode±\else\textpm\fi are entangled for all finite accelerations, whereas, due to the Unruh effect, states \ensuremathΦ\ifmmode±\else\textpm\fi{\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathΦ\ifmmode±\else\textpm\fi lose their entanglement for finite accelerations. This is true for Bell states of two bosonic modes, as well as for Bell states of a bosonic and a fermionic mode. Furthermore, there are also differences in the degradation of entanglement for Bell states of fermionic modes. We reveal the origin of these distinct characteristics of entanglement degradation and discuss the role that is played by particle statistics. Our studies suggest that the behavior of entanglement in accelerated frames strongly depends on the occupation patterns of the constituent states, whose superposition constitutes the entangled state, where especially states \ensuremathΦ\ifmmode±\else\textpm\fi{\mathrm{\ensuremath{\Phi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathΦ\ifmmode±\else\textpm\fi and \ensuremathΨ\ifmmode±\else\textpm\fi{\mathrm{\ensuremath{\Psi}}}^{\ifmmode\pm\else\textpm\fi{}}\ensuremathΨ\ifmmode±\else\textpm\fi exhibit distinct characteristics regarding entanglement degradation. Finally, we point out possible implications of hovering over a black hole for these states.
Entanglement degradation caused by the Unruh effect is discussed for the tripartite GHZ or W states constructed by modes of a non-interacting quantum field viewed by one inertial observer and two uniformly accelerated observers. For fermionic states, the Unruh effect even for infinite accelerations cannot completely remove the entanglement. However, for the bosonic states, the situation is different and the entanglement vanishes asymptotically. Also, the entanglement is studied for the bipartite subsystems. While for the GHZ states all the bipartite subsystems are identically disentangled, for the W states the bipartite subsystems are somewhat entangled, though, this entanglement can be removed for appropriately accelerated observers. Interestingly, logarithmic negativity as a measure for determining the entanglement of one part of the system relative to the other two parts, is not generally the same for different parts. This means that we encounter tripartite systems where each part is differently entangled to the other two parts.
We introduce an arbitrary number of accessible modes when analyzing bipartite entanglement degradation due to Unruh effect between two partners Alice and Rob. Under the single mode approximation (SMA) a fermion field only had a few accessible levels due to Pauli exclusion principle conversely to bosonic fields which had an infinite number of excitable levels. This was argued to justify entanglement survival in the fermionic case in the SMA infinite acceleration limit. Here we relax SMA. Hence, an infinite number of modes are excited as the observer Rob accelerates, even for a fermion field. We will prove that, despite this analogy with the bosonic case, entanglement loss is limited. We will show that this comes from fermionic statistics through the characteristic structure it imposes on the infinite dimensional density matrix for Rob. Surprisingly, the surviving entanglement is independent of the specific maximally entangled state chosen, the kind of fermionic field analyzed, and the number of accessible modes considered. We shall discuss whether this surviving entanglement goes beyond the purely statistical correlations, giving insight concerning the black hole information paradox.
Two observers determine the entanglement between two free bosonic modes by each detecting one of the modes and observing the correlations between their measurements. We show that a state which is maximally entangled in an inertial frame becomes less entangled if the observers are relatively accelerated. This phenomenon, which is a consequence of the Unruh effect, shows that entanglement is an observer-dependent quantity in noninertial frames. In the high acceleration limit, our results can be applied to a nonaccelerated observer falling into a black hole while the accelerated one barely escapes. If the observer escapes with infinite acceleration, the state's distillable entanglement vanishes.
Quantum entanglement is foundational to quantum computation. Yet little is known about how this phenomenon is modified by gravitational effects. One place to begin this study is by consideration of observers in relative acceleration. Here I describe recent work exploring the relationship between quantum entanglement between states shared by such observers. Due to the Unruh effect, the entanglement is degraded and asymptotically reaches a minimum value in the infinite acceleration limit. For bosons this value is zero, but for fermions it is nonzero, in which case quantum information tasks such as teleportation between parties in relative uniform acceleration can always be performed. I discuss the implications of these results for observers in gravitational fields. © 2008 Physics Essay Publications. DOI: XXXX Resume: L’enchevetrement quantique est fondamentale pour le calcul quantique. Pourtant tres peu est connu a propos de comment ce phenomene est modifie par les effets gravitationnels. Une maniere d’entamer cette etude est de considerer des observateurs en acceleration relative. Ici je decris des travaux recents qui explore les relations entre enchevetrement quantique d’etats partages par de tels observateurs. A cause de l’effet dit de Unruh, cet enchevetrement est degrade et atteint asymptotiquement une valeur minimum dans la limite d’une acceleration infinie. Pour les bosons cette valeur est nulle, alors que pour des fermions cette valeur est non zero. Dans ce cas, les operations d’informations quantiques tel que la teleportation entre differentes parties en acceleration relatives peuvent toujours etre etre implementees. Je discusse les implications de ces resultats pour des observateurs dans un champ gravitationel.
We analyze the entanglement between two modes of a free Dirac field as seen by two relatively accelerated parties. The entanglement is degraded by the Unruh effect and asymptotically reaches a nonvanishing minimum value in the infinite acceleration limit. This means that the state always remains entangled to a degree and can be used in quantum information tasks, such as teleportation, between parties in relative uniform acceleration. We analyze our results from the point of view afforded by the phenomenon of entanglement sharing and in terms of recent results in the area of multiqubit complementarity.
A uniformly accelerated observer perceives the Minkowski vacuum as a thermal bath, so acceleration acts as a noise channel on correlations shared with an inertial partner. For a Dirac field in the standard treatment, the resulting map is a one-sided amplitude-damping channel, and entanglement and quantum discord survive at infinite acceleration. We introduce a symmetric Unruh-like map in which the vacuum and the one-particle state both exchange amplitude with the inaccessible Rindler region; for a Bell state it yields a bit-flip channel whose flip probability is the Fermi-Dirac occupation at the Unruh temperature. Using negativity, mutual information, and all six pairwise quantum discords, we find that the entanglement and discord between the inertial observer and the accessible mode vanish together at infinite acceleration, leaving only one bit of classical correlation. These results show that the fate of quantum correlations in noninertial frames depends on the structure of the Minkowski-Rindler map.