Radiative falloff in the background of rotating black hole

Details Radiative falloff in the background of rotating black hole Radiative falloff in the background of rotating black hole

2002-09-27

arxiv.org/abs/gr-qc/0209107v2

Phys.Rev. D67 (2003) 081502

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, 4 Encapsulated PostScript figures; Accepted to Phys. Rev. D (Rapid Communication)

Scientific paper

10.1103/PhysRevD.67.081502

We study numerically the late-time tails of linearized fields with any spin $s$ in the background of a spinning black hole. Our code is based on the ingoing Kerr coordinates, which allow us to penetrate through the event horizon. The late time tails are dominated by the mode with the least multipole moment $\ell$ which is consistent with the equatorial symmetry of the initial data and is equal to or greater than the least radiative mode with $s$ and the azimuthal number $m$.

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