Remarks on the continued-fraction method for computing black-hole quasinormal frequencies and modes

Edward W. Leaver

doi:10.1103/PhysRevD.45.4713

Remarks on the continued-fraction method for computing black-hole quasinormal frequencies and modes

Edward W. Leaver

Phys. Rev. D 45, 4713 – Published 15 June 1992

Abstract

We discuss the stability, accuracy, validity, and convergence of the continued-fraction method for computing black-hole quasinormal frequencies and modes.

Received 17 October 1991

DOI:https://doi.org/10.1103/PhysRevD.45.4713

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Edward W. Leaver

2604 S. Windsor Circle, Salt Lake City, Utah 84106

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Vol. 45, Iss. 12 — 15 June 1992

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Physical Review D

covering particles, fields, gravitation, and cosmology

Remarks on the continued-fraction method for computing black-hole quasinormal frequencies and modes

Edward W. Leaver

Phys. Rev. D 45, 4713 – Published 15 June 1992

Abstract

Authors & Affiliations

References (Subscription Required)

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Access Options

Physical Review D

covering particles, fields, gravitation, and cosmology

Remarks on the continued-fraction method for computing black-hole quasinormal frequencies and modes

Edward W. Leaver

Phys. Rev. D 45, 4713 – Published 15 June 1992

Abstract

Authors & Affiliations

References (Subscription Required)

Issue

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