arXiv Analytics

Sign in

arXiv:gr-qc/9803034AbstractReferencesReviewsResources

On the Completeness of the Quasinormal Modes of the Poeschl-Teller Potential

Horst R. Beyer

Published 1998-03-10Version 1

The completeness of the quasinormal modes of the wave equation with Poeschl-Teller potential is investigated. A main result is that after a large enough time $t_0$, the solutions of this equation corresponding to $C^{\infty}$-data with compact support can be expanded uniformly in time with respect to the quasinormal modes, thereby leading to absolutely convergent series. Explicit estimates for $t_0$ depending on both the support of the data and the point of observation are given. For the particular case of an ``early'' time and zero distance between the support of the data and observational point, it is shown that the corresponding series is not absolutely convergent, and hence that there is no associated sum which is independent of the order of summation.

Comments: 22 pages, 2 figures, submitted to Comm. Math. Phys
Journal: Commun.Math.Phys. 204 (1999) 397-423
Categories: gr-qc
Related articles: Most relevant | Search more
arXiv:gr-qc/9507034 (Published 1995-07-14)
Wave Propagation in Gravitational Systems: Completeness of Quasinormal Modes
arXiv:0908.4247 [gr-qc] (Published 2009-08-28)
Stability, causality and quasinormal modes of cosmic strings and cylinders
arXiv:1201.0208 [gr-qc] (Published 2011-12-31)
Quasinormal modes and entropy spectrum of three dimensional Godel black hole