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

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

2005-10-03

arxiv.org/abs/gr-qc/0510008v3

Phys.Rev. D74 (2006) 028501

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, 4 figures

Scientific paper

10.1103/PhysRevD.74.028501

We confront the predictions of S. Hod, Phys. Rev. D 60, 104053 (1999) for the late-time decay rate of black hole perturbations 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 correction terms, do they take the specific form predicted in Hod's paper? The answer to both questions is ``no.''

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