2014
DOI: 10.1088/0264-9381/31/24/245007
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Onset and decay of the 1 + 1 Hawking–Unruh effect: what the derivative-coupling detector saw

Abstract: We study an Unruh-DeWitt particle detector that is coupled to the proper time derivative of a real scalar field in 1+1 spacetime dimensions. Working within first-order perturbation theory, we cast the transition probability into a regulatorfree form, and we show that the transition rate remains well defined in the limit of sharp switching. The detector is insensitive to the infrared ambiguity when the field becomes massless, and we verify explicitly the regularity of the massless limit for a static detector in… Show more

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Cited by 63 publications
(126 citation statements)
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References 88 publications
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“…For detectors static in the (t, x) coordinates, we have t = τ and the proper time derivative reduces to partial derivative ∂ t . As shown in [28], in addition to removing the dependence of the excitation probability on the infrared cut-off, this coupling also results in an expression for the probability that looks more similar to the (3+1)D case. In the current case, we can see this by the following: the expressions for P (Ω) and X given in Sec.…”
Section: Detector Response and Concurrence In The Presence Of A Boundarymentioning
confidence: 98%
“…For detectors static in the (t, x) coordinates, we have t = τ and the proper time derivative reduces to partial derivative ∂ t . As shown in [28], in addition to removing the dependence of the excitation probability on the infrared cut-off, this coupling also results in an expression for the probability that looks more similar to the (3+1)D case. In the current case, we can see this by the following: the expressions for P (Ω) and X given in Sec.…”
Section: Detector Response and Concurrence In The Presence Of A Boundarymentioning
confidence: 98%
“…While we have focused the present paper on static flat spacetimes and to quantum states that are invariant under translations in the Killing time, there would be scope for examining the detector coupled to the Dirac field in more general spacetimes and for more general quantum states, including collapsing star spacetimes [34] and their flat "moving mirror" counterparts [5,18], or spatially homogeneous cosmologies, where Dirac's equation can be solved by separation of variables [35]. For example, if a cosmological spacetime has a de Sitter era, exactly or approximately, how does the detector register the associated Gibbons-Hawking temperature [36]?…”
Section: Discussionmentioning
confidence: 99%
“…Despite its mathematical simplicity, this modelling captures the core features of the dipole interaction by which atomic orbitals couple to the electromagnetic field [3,4]. In the special case of a uniformly linearly accelerated observer coupled to a field in its Minkowski vacuum, detector analyses have provided significant evidence that the Unruh effect [1], the thermal response of the observer, occurs whenever the interaction time is long, the interaction switch-on and switch-off are sufficiently slow and the back-reaction of the observer on the quantum field remains small [1,2,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19].…”
Section: Introductionmentioning
confidence: 99%
“…with the response function is given by (22). As it is explained in [21] that this quantity (52) is well defined as a function where the pole atȗ = 0 can be avoided by subtracting the extra factor (A similar regularised Wightman function for (1 + 1) dimensional case has been advocated in [28] for a derivative type coupling).…”
Section: A Detector Responsementioning
confidence: 99%