Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University
Phys. Rev. D 105(8), 22 (2022)
We consider the response of an Unruh-DeWitt detector near an extremal charged black hole, modeling the near-horizon region of this extremal spacetime by the Bertotti-Robinson spacetime. The advantage of employing the Bertotti-Robinson limit is that the two-point functions for a massless scalar field are obtainable in closed form for the field in a number of quantum states of interest. We consider the detector coupled to a massless field in both the Boulware vacuum state and arbitrary thermal states, including the Hartle-Hawking state, and analyze the detector’s response for a broad range of trajectories. Particular attention is paid to the thermalization of the detector, the anti-Unruh and anti-Hawking effect.
@article{UTF914,
author = {Conroy, A. and Taylor, P.},
title = {{Response of an Unruh-DeWitt detector near an extremal black hole}},
journal = {Phys. Rev. D},
volume = {105},
number = {8},
pages = {22},
year = {2022},
month = {4},
doi = {10.1103/PhysRevD.105.085001},
}