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Phys. Rev. D 74, 028501 (2006) [4 pages]

Comment on "High-order contamination in the tail of gravitational collapse"

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Alexander Z. Smith¹ and Lior M. Burko^1,2
¹Department of Physics and Astronomy, Bates College, Lewiston, Maine 04240, USA
²Department of Physics, University of Alabama in Huntsville, Huntsville, Alabama 38599, USA

Received 3 October 2005; published 21 July 2006

Weconfront the predictions of S. Hod [Phys. Rev. D 60,104053 (1999)] for the late-time decay rate of black holeperturbations with numerical data. Specifically, we ask two questions: First,are corrections to the Price tail dominated by logarithmic terms,as predicted by Hod? Second, if there were logarithmic correctionterms, do they take the specific form predicted in Hod'spaper? The answer to both questions is "no."

©2006 The American Physical Society

URL:	http://link.aps.org/doi/10.1103/PhysRevD.74.028501
DOI:	10.1103/PhysRevD.74.028501
PACS:	04.70.Bw; 04.25.Nx; 04.30.Nk 04.70.Bw Classical black holes 04.25.Nx Post-Newtonian approximation; perturbation theory; related approximations 04.30.Nk Gravitational wave propagation and interactions YEAR: 2006

See Also

High-order contamination in the tail of gravitational collapse
Shahar Hod
Phys. Rev. D 60, 104053 (1999)

REFERENCES (10)

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R. H. Price, Phys. Rev. D 5, 2419 (1972).
E. W. Leaver, Phys. Rev. D 34, 384 (1986).
E. S. C. Ching, P. T. Leung, W. M. Suen, and K. Young, Phys. Rev. D 52, 2118 (1995).
C. Gundlach, R. H. Price, and J. Pullin, Phys. Rev. D 49, 883 (1994);

L. M. Burko and A. Ori, Phys. Rev. D 56, 7820 (1997).
L. M. Burko and G. Khanna, Phys. Rev. D 67, 081502 (2003).
M. A. Scheel, A. L. Erickcek, L. M. Burko, L. E. Kidder, H. P. Pfeiffer, and S. A. Teukolsky, Phys. Rev. D 69, 104006 (2004).
R. H. Price and L. M. Burko, Phys. Rev. D 70, 084039 (2004).
S. Hod, Phys. Rev. D 60, 104053 (1999).

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High-order contamination in the tail of gravitational collapse
Shahar Hod
Phys. Rev. D 60, 104053 (1999)

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