Darboux transformation in black hole perturbation theory

Kostas Glampedakis, Aaron D. Johnson, and Daniel Kennefick
Phys. Rev. D 96, 024036 – Published 24 July 2017

Abstract

The Darboux transformation between ordinary differential equations is a 19th century technique that has seen wide use in quantum theory for producing exactly solvable potentials for the Schrödinger equation with specific spectral properties. In this paper we show that the same transformation appears in black hole theory, relating, for instance, the Zerilli and Regge-Wheeler equations for axial and polar Schwarzschild perturbations. The transformation reveals these two equations to be isospectral, a well known result whose method has been repeatedly reintroduced under different names. We highlight the key role that the so-called algebraically special solutions play in the black hole Darboux theory and show that a similar relation exists between the Chandrasekhar-Detweiler equations for Kerr perturbations. Finally, we discuss the limitations of the method when dealing with long-range potentials and explore the possibilities offered by a generalized Darboux transformation.

  • Received 20 February 2017

DOI:https://doi.org/10.1103/PhysRevD.96.024036

© 2017 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Kostas Glampedakis1,2,*, Aaron D. Johnson3, and Daniel Kennefick3,4

  • 1Departamento de Física, Universidad de Murcia, Murcia E-30100, Spain
  • 2Theoretical Astrophysics, University of Tübingen, Auf der Morgenstelle 10, Tübingen D-72076, Germany
  • 3Department of Physics, University of Arkansas, Fayetteville, Arkansas 72701, USA
  • 4Arkansas Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, Arkansas 72701, USA

  • *kostas@um.es

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Issue

Vol. 96, Iss. 2 — 15 July 2017

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