Late-time dynamics of scalar fields on rotating black hole backgrounds

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 60, Issue 10, 1999, Pages

  Krivan, William ^a  

^a UNIVERSITY OF UTAH   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 18144367729     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.101501     Document Type: Article

References (11)

1. S.A. Teukolsky, Phys. Rev. Lett. 29, 1114 (1972).
2. R.H. Price, Phys. Rev. D 5, 2419 (1972).
3. E.W. Leaver, Phys. Rev. D 34, 384 (1986).
4. C. Gundlach, R.H. Price, and J. Pullin, Phys. Rev. D 49, 883 (1994).
5. E.S.C. Ching, P.T. Leung, W.M. Suen, and K. Young, Phys. Rev. Lett. 74, 2414 (1995).
6. N. Andersson, Phys. Rev. D 55, 468 (1997).
7. L. Barack, Phys. Rev. D 59, 044017 (1999).
8. W. Krivan, P. Laguna, and P. Papadopoulos, Phys. Rev. D 54, 4728 (1996).
9. Please note that Fig. 6 from 8 should exhibit the same qualitative features as Fig. 22. As a careful error analysis in connection with the work published in this paper has shown, Fig. 6 in 8 does not correctly describe the transition from the (Formula presented) to the (Formula presented) multipole (due to a relatively coarse grid spacing in the Boyer-Lindquist (Formula presented) coordinate).
10. L. Barack and A. Ori, Phys. Rev. Lett. 82, 4388 (1999).
11. S. Hod, Phys. Rev. D (to be published), gr-qc/9902072.