Quasi-Normal Modes of Stars and Black Holes

Author:

Kokkotas Kostas D.,Schmidt Bernd G.

Publisher

Springer Science and Business Media LLC

Subject

Physics and Astronomy (miscellaneous)

Reference215 articles.

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2. Abrahams, A.M., and Price, R.H., “Applying black hole perturbation theory to numerically generated space-times.”, Phys. Rev. D, 53, 1963–1971, (1996). For a related online version see: A.M. Abrahams, et al., “Applying black hole perturbation theory to numerically generated spacetimes”, (1995), [Online Los Alamos Archive Preprint]: cited on 28 August 1995, http://xxx.lanl.gov/abs/gr-qc/9508059. 5

3. Abrahams, A.M., Shapiro, S.L., and Teukolsky, S.A., “Calculation ofgrav-itational waveforms from black hole collisions and disk collapse: Applying perturbation theory to numerical scpacetimes”, Phys. Rev. D, 51, 42954301, (1995). For a related online version see: A.M. Abrahams, et al., “Calculation of gravitational wave forms from black hole collisions and disk collapse: Applying perturbation theory to numerical spacetimes”, (1994), [Online Los Alamos Archive Preprint]: cited on 29 August 1994, http://xxx.lanl.gov/abs/gr-qc/9408036. 5

4. Albererio, S., Ferreira, L.S., and Streit, L., eds., Lecture Notes in Physics 211 Proceedings Bielefeld, (Springer-Verlag, Berlin, 1984). 9

5. Allen, G., Andersson, N., Kokkotas, K.D., and Schutz, B.F., “Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star”, Phys. Rev. D, 58, 124012, (1998). For a related online version see: G. Allen, et al., “Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star”, (1997), [Online Los Alamos Archive Preprint]: cited on 8 April 1997, http://xxx.lanl.gov/abs/gr-qc/9704023. 4.1, 4.1, 5.2, 5.4, 6.1.1, 4

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