Diamond's temperature: Unruh effect for bounded trajectories and thermal time hypothesis

作者：Martinetti P^*; Rovelli C

来源：Classical and Quantum Gravity, 2003, 20(22): 4919-4931.

DOI：10.1088/0264-9381/20/22/015

We study the Unruh effect for an observer with a finite lifetime, using the thermal time hypothesis. The thermal time hypothesis maintains that: (i) time is the physical quantity determined by the flow defined by a state over an observable algebra and (ii) when this flow is proportional to a geometric flow in spacetime, the temperature is the ratio between flow parameter and proper time. An eternal accelerated Unruh observer has access to the local algebra associated with a Rindler wedge. The flow defined by the Minkowski vacuum of a field theory over this algebra is proportional to a flow in spacetime and the associated temperature is the Unruh temperature. An observer with a finite lifetime has access to the local observable algebra associated with a finite spacetime region called a 'diamond'. The flow defined by the Minkowski vacuum of a (four-dimensional, conformally invariant) quantum field theory over this algebra is also proportional to a flow in spacetime. The associated temperature generalizes the Unruh temperature to finite lifetime observers. Furthermore, this temperature does not vanish even in the limit in which the acceleration is zero. The temperature associated with an inertial observer with lifetime T, which we denote as 'diamond's temperature', is T-D = 2 (h) over bar /7pik(b)T. This temperature is related to the fact that a finite lifetime observer does not have access to all the degrees of freedom of the quantum field theory. However, we do not attempt to provide any physical interpretation of our proposed assignment of a temperature.

• 出版日期2003-11-21