Evolving test fields in a black-hole geometry

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 2, 1997, Pages 468-479

  Andersson, Nils ^a  

^a WASHINGTON UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001168617     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.468     Document Type: Article

References (35)

1. S. Chandrasekhar, The Mathematical Theory of Black Holes (Oxford University Press, New York, 1983).
2. N. Andersson, in Physics of Black Holes, by I. D. Novikov and V. Frolov (Kluwer Academic, Boca Raton, FL, 1996), Chap. 4.
3. E. W. Leaver, Phys. Rev. D34, 384 (1986).
4. N. Andersson, Phys. Rev. D51, 353 (1995).
5. C. T. Cunningham, R. H. Price, and V. Moncrief, Astrophys. J.224, 643 (1978).
6. C. T. Cunningham, R. H. Price, and V. Moncrief, Astrophys. J.230, 870 (1979).
7. E. Seidel, Phys. Rev. D42, 1884 (1990).
8. E. Seidel, Phys. Rev. D44, 950 (1991).
9. R. H. Price, Phys. Rev. D5, 2419 (1972).
10. R. H. Price, Phys. Rev. D5, 2439 (1972).
11. R. H. Price and J. Pullin, Phys. Rev. Lett.72, 3297 (1994).
12. C. V. Vishveshwara, Nature (London)227, 936 (1970).
13. Y. Sun and R. H. Price, Phys. Rev. D38, 1040 (1988).
14. C. Gundlach, R. H. Price, and J. Pullin, Phys. Rev. D49, 883 (1994).
15. C. Gundlach, R. H. Price, and J. Pullin, Phys. Rev. D49, 890 (1994).
16. E. S. C. Ching, P. T. Leung, W. M. Suen, and K. Young, Phys. Rev. D52, 2118 (1995).
17. H-P. Nollert, Phys. Rev. D47, 5253 (1993).
18. N. Andersson, Class. Quantum Grav.10, L61 (1993).
19. E. W. Leaver, Proc. R. Soc. LondonA402, 285 (1985).
20. N. Andersson, Proc. R. Soc. LondonA439, 47 (1992).
21. N. Andersson and S. Linnæus, Phys. Rev. D46, 4179 (1992).
22. H-P. Nollert and B. G. Schmidt, Phys. Rev. D45, 2617 (1992).
23. B. F. Schutz and C. M. Will, Astrophys. J.291, L33 (1985).
24. K. S. Thorne, in Magic without Magic: John Archibald Wheeler, edited by J. Klauder (Freeman, San Francisco, 1972), p. 231.
25. This low-frequency approximation can be used only for (Formula presented). The special case of (Formula presented) must be considered separately. This has been done by Ching et al. 16.
26. J. A. H. Futterman, F. A. Handler, and R. A. Matzner, Scattering from Black Holes (Cambridge University Press, Cambridge, England, 1988).
27. M. Abramowitz and I. A. Stegun, Handbook of Mathematical Functions (Dover, New York, 1970).
28. H. Liu and B. Mashhoon, Class. Quantum Grav.13, 233 (1996).
29. I. S. Gradshteyn and I. M. Ryzhik, Table of Integrals, Series and Products (Academic, London, 1980).
30. R. Capon (private communication).
31. W. Krivan, P. Laguna, and P. Papadopoulos, Phys. Rev. D54, 4728 (1996).
32. S. A. Teukolsky, Astrophys. J.185, 635 (1973).
33. E. Seidel, Class. Quantum Grav.6, 1057 (1989).
34. S. Chandrasekhar, Proc. R. Soc. LondonA343, 289 (1975).
35. J. M. Bardeen and W. H. Press, J. Math. Phys. (N.Y.)14, 7 (1973).