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ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

ENTANGLEMENT OF GAUSSIAN STATES Gerardo Adesso

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CHAPTER 14<br />

Gaussian entanglement sharing in<br />

non-inertial frames<br />

In the study of most quantum information tasks such as teleportation and quantum<br />

cryptography, non-relativistic observers share entangled resources to perform their<br />

experiments [163]. Apart from a few studies [61, 88, 6, 14, 7, 4], most works<br />

on quantum information assume a world without gravity where space-time is flat.<br />

But the world is relativistic and any serious theoretical study must take this into<br />

account. It is therefore of fundamental interest to revise quantum information<br />

protocols in relativistic settings [179]. It has been shown that relativistic effects<br />

on quantum resources are not only quantitatively important but also induce novel,<br />

qualitative features [88, 6, 14, 4]. For example, it has been shown that the dynamics<br />

of space-time can generate entanglement [14]. This, in principle, would have a<br />

consequence in any entanglement-based protocol performed in curved space-time.<br />

Relativistic effects have also been found to be relevant in a flat spacetime where the<br />

entanglement measured by observers in relative acceleration is observer-dependent<br />

since it is degraded by the Unruh effect [88, 6, 4]. In the infinite acceleration limit,<br />

the entanglement vanishes for bosons [88, 4] and reaches a non-vanishing minimum<br />

for fermions [6]. This degradation on entanglement results in the loss of fidelity of<br />

teleportation protocols which involve observers in relative acceleration [7].<br />

Understanding entanglement in a relativistic framework is not only of interest to<br />

quantum information. Relativistic entanglement plays an important role in black<br />

hole entropy [26, 46, 187] and in the apparent loss of information in black holes<br />

[228], one of the most challenging problems in theoretical physics at the moment<br />

[108, 109]. Understanding the entanglement between modes of a field close to the<br />

horizon of a black hole might help to understand some of the key questions in black<br />

hole thermodynamics and their relation to information.<br />

In this Chapter, based on Ref. [GA20], we interpret the loss of bipartite entanglement<br />

between two modes of a scalar field in non-inertial frames as an effect<br />

of entanglement redistribution. We consider two observers, each with a detector<br />

sensitive to a single mode. The observers make measurements on the field and look<br />

for correlations to determine the degree to which the field modes are entangled.<br />

Suppose that the observers are inertial and that the two field modes measured are<br />

entangled to a given degree. The state will appear less entangled if the observers<br />

move with uniform acceleration in a non-inertial frame [88]. This is because each inertial<br />

mode becomes a two-mode squeezed state in non-inertial coordinates [63, 233].<br />

Therefore, the two-mode entangled state in the inertial frame becomes a three-mode<br />

state when one observer is in uniform acceleration and a four-mode state if both<br />

observers are accelerated. The observers moving with uniform acceleration have<br />

235

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