Unruh effect for inertial observers through vacuum correlations
Kinjalk Lochan, Sumanta Chakraborty, T. Padmanabhan

TL;DR
This paper demonstrates that inertial observers in a flat spacetime region can detect a thermal quantum field state due to vacuum correlations, revealing a dynamic Unruh-like effect without acceleration or causal connection to the radiation source.
Contribution
It shows that vacuum correlations can produce a thermal perception for inertial observers in a collapsing black hole model, extending the understanding of the Unruh effect beyond accelerated frames.
Findings
Inertial observers in flat spacetime perceive thermal radiation.
Thermal state arises from quantum correlations outside the past light cone.
Observers detect the same temperature as accelerated Unruh observers.
Abstract
We study a dynamic version of the Unruh effect in a two dimensional collapse model forming a black hole. In this two-dimensional collapse model a scalar field coupled to the dilaton gravity, moving leftwards, collapses to form a black hole. There are two sets of asymptotic () observers, around and . The observers at the right null infinity witness a thermal flux of radiation associated with time dependent geometry leading to a black hole formation and its subsequent Hawking evaporation, in an expected manner. We show that even the observers at left null infinity find themselves in thermal ambiance, without experiencing any change of spacetime geometry all along their trajectories. They remain as inertial observers in a \emph{flat} region of spacetime where curvature tensor identically vanishes in a portion of full spacetime. These observers find the…
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