Master equations and stability of Einstein-Maxwell-scalar black holes

Abstract We derive master equations for linear perturbations in Einstein-Maxwell scalar theory, for any spacetime dimension D and any background with a maximally symmetric n = (D - 2)-dimensional spatial component. This is done by expressing all fluctuations analytically in terms of several master s...

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Bibliographic Details
Main Authors: Aron Jansen, Andrzej Rostworowski, Mieszko Rutkowski
Format: Article
Language:English
Published: SpringerOpen 2019-12-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP12(2019)036