Skip to main content
Log in

Decay of Solutions of the Wave Equation in the Kerr Geometry

  • Published:
Communications in Mathematical Physics Aims and scope Submit manuscript

An Erratum to this article was published on 18 March 2008

Abstract

We consider the Cauchy problem for the massless scalar wave equation in the Kerr geometry for smooth initial data compactly supported outside the event horizon. We prove that the solutions decay in time in L loc. The proof is based on a representation of the solution as an infinite sum over the angular momentum modes, each of which is an integral of the energy variable ω on the real line. This integral representation involves solutions of the radial and angular ODEs which arise in the separation of variables.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. Cardoso, V., Yoshida, S.: Superradiant instabilities of rotating black branes and strings. JHEP 0507, 009 (2005)

    Article  ADS  MathSciNet  Google Scholar 

  2. Chandrasekhar, S.: The mathematical theory of black holes. Oxford: Oxford University Press, 1983

  3. De Alfaro, V., Regge, T.: Potential Scattering. Amsterdam: North-Holland Publishing Company, 1965

  4. Finster, F., Kamran, N., Smoller, J., Yau, S.T.: The long-time dynamics of Dirac particles in the Kerr-Newman black hole geometry. Adv. Theor. Math. Phys. 7, 25–52 (2003)

    MathSciNet  Google Scholar 

  5. Finster, F., Kamran, N., Smoller, J., Yau, S.T.: An integral spectral representation of the propagator for the wave equation in the Kerr geometry, Commun. Math. Phys. 260, no.2, 257–298 (2005)

    Google Scholar 

  6. Finster, F., Schmid, H.: Spectral estimates and non-selfadjoint perturbations of spheroidal wave operators. http://atxiv.org/list/math-ph/0405010 to appear in Grelle's Journal (2006)

  7. Kay, B., Wald, R.: Linear stability of Schwarzschild under perturbations which are nonvanishing on the bifurcation 2-sphere. Classical Quantum Gravity 4, 893–898 (1987)

    Article  ADS  MATH  MathSciNet  Google Scholar 

  8. Press, W.H., Teukolsky, S.A.: Perturbations of a rotating black hole. II. Dynamical stability of the Kerr metric. Astrophys.J. 185, 649 (1973)

    Google Scholar 

  9. Price, R.H.: Nonspherical perturbations of relativistic gravitational collapse I, scalar and gravitational perturbations. Phys. Rev. D (3) 5, 2419–2438 (1972)

    Google Scholar 

  10. Whiting, B.: Mode stability of the Kerr black hole. J. Math. Phys 30, 1301–1305 (1989)

    Article  ADS  MATH  MathSciNet  Google Scholar 

  11. Regge, T., Wheeler, J.A.: Stability of the Schwarzschild singularity. Phys. Rev. (2) 108, 1063–1069 (1957)

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to F. Finster.

Additional information

Communicated by G.W. Gibbons

Research supported in part by the Deutsche Forschungsgemeinschaft.

Research supported by NSERC grant #RGPIN 105490-2004.

Research supported in part by the NSF, Grant No. DMS-010-3998.

Research supported in part by the NSF, Grant No. 33-585-7510-2-30.

An erratum to this article is available at http://dx.doi.org/10.1007/s00220-008-0458-9.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Finster, F., Kamran, N., Smoller, J. et al. Decay of Solutions of the Wave Equation in the Kerr Geometry. Commun. Math. Phys. 264, 465–503 (2006). https://doi.org/10.1007/s00220-006-1525-8

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00220-006-1525-8

Keywords

Navigation