no code implementations • 12 Mar 2021 • Michael R. R. Good, Alessio Lapponi, Orlando Luongo, Stefano Mancini
Motivated by the fact that the null-shell of a collapsing black hole can be described by a perfectly reflecting accelerating mirror, we investigate an extension of this model to mirror semi-transparency and derive a general implicit expression for the corresponding Bogoliubov coefficients.
General Relativity and Quantum Cosmology Quantum Physics