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      Unruh-DeWitt detector response across a Rindler firewall is finite

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          Abstract

          We investigate a two-level Unruh-DeWitt detector coupled to a massless scalar field or its proper time derivative in \((1+1)\)-dimensional Minkowski spacetime, in a quantum state whose correlation structure across the Rindler horizon mimics the stationary aspects of a firewall that Almheiri et al have argued to ensue in an evaporating black hole spacetime. Within first-order perturbation theory, we show that the detector's response on falling through the horizon is sudden but finite. The difference from the Minkowski vacuum response is proportional to \(\omega^{-2}\ln(|\omega|)\) for the non-derivative detector and to \(\ln(|\omega|)\) for the derivative-coupling detector, both in the limit of a large energy gap \(\omega\) and in the limit of adiabatic switching. Adding to the quantum state high Rindler temperature excitations behind the horizon increases the detector's response proportionally to the temperature; this situation has been suggested to model the energetic curtain proposal of Braunstein et al. We speculate that the \((1+1)\)-dimensional derivative-coupling detector may be a good model for a non-derivative detector that crosses a firewall in \(3+1\) dimensions.

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          Violating Bell's inequalities in the vacuum

          , , (2003)
          We employ an approach wherein vacuum entanglement is directly probed in a controlled manner. The approach consists of having a pair of initially nonentangled detectors locally interact with the field for a finite duration, such that the two detectors remain causally disconnected, and then analyzing the resulting detector mixed state. It is demonstrated that the correlations between arbitrarily far-apart regions of the vacuum of a relativistic free scalar field cannot be reproduced by a local hidden-variable model, and that as a function of the distance L between the regions, the entanglement decreases at a slower rate than exp(-(L/cT)^3).
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            Stochastic Theory of Accelerated Detectors in a Quantum Field

            We analyze the statistical mechanical properties of n-detectors in arbitrary states of motion interacting with each other via a quantum field. We use the open system concept and the influence functional method to calculate the influence of quantum fields on detectors in motion, and the mutual influence of detectors via fields. We discuss the difference between self and mutual impedance and advanced and retarded noise. The mutual effects of detectors on each other can be studied from the Langevin equations derived from the influence functional, as it contains the backreaction of the field on the system self-consistently. We show the existence of general fluctuation- dissipation relations, and for trajectories without event horizons, correlation-propagation relations, which succinctly encapsulate these quantum statistical phenomena. These findings serve to clarify some existing confusions in the accelerated detector problem. The general methodology presented here could also serve as a platform to explore the quantum statistical properties of particles and fields, with practical applications in atomic and optical physics problems.
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              Hadamard renormalization of the stress-energy tensor for a quantized scalar field in a general spacetime of arbitrary dimension

              We develop the Hadamard renormalization of the stress-energy tensor for a massive scalar field theory defined on a general spacetime of arbitrary dimension. Our formalism could be helpful in treating some aspects of the quantum physics of extra spatial dimensions. More precisely, for spacetime dimension up to six, we explicitly describe the Hadamard renormalization procedure and for spacetime dimension from seven to eleven, we provide the framework permitting the interested reader to perform this procedure explicitly in a given spacetime. We complete our study (i) by considering the ambiguities of the Hadamard renormalization of the stress-energy tensor and the corresponding ambiguities for the trace anomaly, (ii) by providing the expressions of the gravitational counterterms involved in the renormalization process (iii) by discussing the connections between Hadamard renormalization and renormalization in the effective action. All our results are expanded on standard bases for Riemann polynomials constructed from group theoretical considerations and thus given on irreducible forms.
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                Author and article information

                Journal
                2014-07-23
                2015-08-09
                Article
                10.1007/JHEP09(2014)142
                1407.6299
                2115991d-c0cb-4465-bbcf-68279b2c5fd6

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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                Custom metadata
                JHEP 1409 (2014) 142
                24 pages. v4: post-JHEP correction in the parity description of Delta F in Section 5
                hep-th gr-qc quant-ph

                Quantum physics & Field theory,General relativity & Quantum cosmology,High energy & Particle physics

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