Revisiting the quasinormal modes of the Schwarzschild black hole: Numerical analysis

Abstract We revisit the problem of calculating the quasinormal modes of spin 0, 1/2, 1, 3/2, 2, and spin 5/2 fields in the asymptotically flat Schwarzschild black hole spacetime. Our aim is to investigate the problem from the numerical point of view, by comparing some numerical methods available in...

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Bibliographic Details
Main Authors: Luis A. H. Mamani, Angel D. D. Masa, Lucas Timotheo Sanches, Vilson T. Zanchin
Format: Article
Language:English
Published: SpringerOpen 2022-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-022-10865-1