Black Hole Decay and Quantum Instantons
Donsu Bak, Sang Pyo Kim, Sung Ku Kim, Kwang-Sup Soh, Jae Hyung Yee

TL;DR
This paper explores the analytic structure of the S-matrix in quantum gravity, revealing that its poles correspond to quantum instantons related to black hole quasi-normal modes, offering insights into black hole decay.
Contribution
It introduces the concept of quantum instantons as solutions from the Euclidean Wheeler-DeWitt equation linked to black hole quasi-normal modes.
Findings
Poles in the S-matrix correspond to quantum instantons.
Wave functions satisfy boundary conditions similar to black hole quasi-normal modes.
Quantum instantons are related to bounded states in Euclidean quantum gravity.
Abstract
We study the analytic structure of the S-matrix which is obtained from the reduced Wheeler-DeWitt wave function describing spherically symmetric gravitational collapse of massless scalar fields. The complex simple poles in the S-matrix lead to the wave functions that satisfy the same boundary condition as quasi-normal modes of a black hole, and correspond to the bounded states of the Euclidean Wheeler-DeWitt equation. These wave function are interpreted as quantum instantons.
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