Black Hole - Moving Mirror I: An Exact Correspondence
Paul R. Anderson, Michael R.R. Good, and Charles R. Evans

TL;DR
This paper establishes an exact mathematical correspondence between a specific moving mirror trajectory in (1+1)D spacetime and a black hole formation scenario, providing explicit Bogolubov coefficients and discussing potential generalizations to higher dimensions.
Contribution
It introduces a novel exact correspondence linking moving mirror trajectories to black hole formation, with explicit calculations of Bogolubov coefficients and discussion of higher-dimensional extensions.
Findings
Exact Bogolubov coefficients derived for the correspondence
Demonstrated equivalence between mirror trajectory and black hole spacetime
Discussed potential generalization to (3+1)D black holes
Abstract
An exact correspondence is shown between a new moving mirror trajectory in (1+1)D and a spacetime in (1+1)D in which a black hole forms from the collapse of a null shell. It is shown that the Bogolubov coefficients between the "in" and "out" states are identical and the exact Bogolubov coefficients are displayed. Generalization to the (3+1)D black hole case is discussed.
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