Waiting for Unruh

Abstract

How long does a uniformly accelerated observer need to interact with a quantum field in order to record thermality in the Unruh temperature? We address this question for a pointlike Unruh-DeWitt detector, coupled linearly to a real Klein-Gordon field of mass $m\ge 0$ and treated within first order perturbation theory, in the limit of large detector energy gap $E_{\text{gap}}$. We first show that when the interaction duration $\Delta T$ is fixed, thermality in the sense of detailed balance cannot hold as $E_{\text{gap}}\to \infty$, and this property generalises from the Unruh effect to any Kubo-Martin-Schwinger state satisfying certain technical conditions. We then specialise to a massless field in four spacetime dimensions and show that detailed balance does hold when $\Delta T$ grows as a power-law in $E_{\text{gap}}$ as $E_{\text{gap}}\to \infty$, provided the switch-on and switch-off intervals are stretched proportionally to $\Delta T$ and the switching function has sufficiently strong Fourier decay. By contrast, if $\Delta T$ grows by stretching a plateau in which the interaction remains at constant strength but keeping the duration of the switch-on and switch-off intervals fixed, detailed balance at $E_{\text{gap}}\to \infty$ requires $\Delta T$ to grow faster than any polynomial in $E_{\text{gap}}$, under mild technical conditions. These results also hold for a static detector in a Minkowski heat bath. The results limit the utility of the large $E_{\text{gap}}$ regime as a probe of thermality in time-dependent versions of the Hawking and Unruh effects, such as an observer falling into a radiating black hole. They may also have implications on the design of prospective experimental tests of the Unruh effect.

29 pages. v2: minor clarifications, references added, typos corrected

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