arXiv · 2507.16493
Transients in black hole perturbation theory
Abstract
Black hole quasinormal modes arise as eigenmodes of a non-normal Hamiltonian and consequently they do not obey orthogonality relations with respect to commonly used inner products, for example, the energy inner product. A direct consequence of this is the appearance of transient phenomena. This review summarises current developments on the topic, both in frequency- and time-domain. In particular, we discuss the appearance of i) transient plateaus: arbitrarily long-lived sums of quasinormal modes, corresponding to localised energy packets near the future horizon; ii) transient growth, with the latter either appearing in the vicinity of black hole phase transitions or in the context of higher-derivative Sobolev norms.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Jérémy Besson, Javier Carballo, Christiana Pantelidou, Benjamin Withers. 2025-07-22. Transients in black hole perturbation theory. https://doi.org/10.3389/fphy.2025.1638583
Cite the original work for its findings. Save a collection to share your selection of sources.