The uncertainty principle bounds our ability to simultaneously predict two
incompatible observables of a quantum particle. Assisted by a quantum memory to
store the particle, this uncertainty could be reduced and quantified by a new
Entropic Uncertainty Relation (EUR). In this Letter, we explore how the
relativistic motion of the system would affect the EUR in two sample scenarios.
First, we show that the Unruh effect of an accelerating particle would surely
increase the uncertainty if the system and particle entangled initially. On the
other hand, the entanglement could be generated from nonuniform motion once the
Unruh decoherence is prevented by utilizing the cavity. We show that, in a
uncertainty game between an inertial cavity and a nonuniformly accelerated one,
the uncertainty evolves periodically with respect to the duration of
acceleration segment. Therefore, with properly chosen cavity parameters, the
uncertainty bound could be protected. Implications of our results for
gravitation are also discussed.Comment: 7 pages, 3 figure
We explore the entropic uncertainty relation in the curved background outside
a Schwarzschild black hole, and find that Hawking radiation introduces a
nontrivial modification on the uncertainty bound for particular observer,
therefore it could be witnessed by proper uncertainty game experimentally. We
first investigate an uncertainty game between a free falling observer and his
static partner holding a quantum memory initially entangled with the quantum
system to be measured. Due to the information loss from Hawking decoherence, we
find an inevitable increase of the uncertainty on the outcome of measurements
in the view of static observer, which is dependent on the mass of the black
hole, the distance of observer from event horizon, and the mode frequency of
quantum memory. To illustrate the generality of this paradigm, we relate the
entropic uncertainty bound with other uncertainty probe, e.g., time-energy
uncertainty. In an alternative game between two static players, we show that
quantum information of qubit can be transferred to quantum memory through a
bath of fluctuating quantum fields outside the black hole. For a particular
choice of initial state, we show that the Hawking decoherence cannot counteract
entanglement generation after the dynamical evolution of system, which triggers
an effectively reduced uncertainty bound that violates the intrinsic limit
$-\log_2c$. Numerically estimation for a proper choice of initial state shows
that our result is comparable with possible real experiments. Finally, a
discussion on the black hole firewall paradox in the context of entropic
uncertainty relation is given.Comment: 11 pages, 2figures. Minor typos corrected, references and comment on
the black hole firewall added. Matches the version to appear in Physics
Letters
We investigate the quantum estimation on the Hubble parameter of an expanding de Sitter space by quantum metrological techniques. By exploring the dynamics of a freely falling Unruh-DeWitt detector, which interacts with a scalar field coupling to curvature, we calculate the Fisher information (FI) and quantum Fisher information (QFI) for the detector, which bound the highest precision of the estimation on Hubble parameter. In standard Bunch-Davies vacuum, we show that the maxima of FI/QFI are located for particular initial state of probe. Beside its dependence on the evolving time of detector and the energy spacing of atom ω, we show that the maxima of FI/QFI can be significantly enhanced once a proper coupling of scalar field to curvature is chosen. For instance, we show numerically that the estimation in the scenario with minimally/nearly minimally coupling scalar field can always outperform that with conformally coupling scalar field, corresponding to a higher FI/QFI in estimation. Moreover, we find that for general α−vacua of de Sitter space, a further improvement of estimation can be achieved, attributed to the squeezed nature of α−vacua that heavily constrains the measurement uncertainty. Some implications of our results are also discussed.
With the help of the Drinfeld twist or factorizing F-matrix for the eight-vertex SOS model, we obtain the explicit determinant expression of the partition function of the eight-vertex model with a generic non-diagonal reflecting end and domain wall boundary condition. Our result shows that, contrary to the eight-vertex model without a reflection end, the partition function can be expressed as a single determinant.
An analysis of Hawking radiation about apparent horizon in a FRW universe is performed by using the method developed in the paper (Banerjee, Majhi in JHEP 06:095 2008), in which the Hawking radiation of a black hole is treated as the quantum tunneling by Hamilton-Jacobi method beyond semiclassical approximation and then all the higher order quantum corrections can be given out. In our analysis, the Kodama vector instead of the Killing vector to define the energy of the particle plays a key role. We present our analysis under the Friedmann-Robertson-Walker like coordinate system and the much-like to Painlevé coordinate system respectively. The result show that the formulized procedure can be extended to fully analyse the Hawking radiation of a dynamical system.
We investigate the quantum teleportation between a conformal detector Alice
and an inertial detector Bob in de Sitter space in two schemes, (i) one uses
free scalar modes and (ii) one utilizes cavity to store qubit. We show that the
fidelity of the teleportation is degraded for Bob in both cases. While the
fidelity-loss is due to the Gibbons-Hawking effect associated with his
cosmological horizon in the scheme (i), the entanglement decreases in the
scheme (ii) because the ability to entangle the cavities is reduced by the
spacetime curvature. With a cutoff at Planck-scale, comparing with the standard
Bunch-Davies choice, we also show that the possible Planckian physics cause
extra modifications to the fidelity of the teleportation protocol in both
schemes.Comment: 6 pages, 2 figures, typos corrected. To appear in Phys. Lett.
With the help of the F-basis provided by the Drinfeld twist or factorizing F-matrix for the open XXZ spin chain with non-diagonal boundary terms, we obtain the determinant representations of the scalar products of Bethe states of the model.
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