2000/12/29 by S. Husa, Sascha Husa, Manuela Campanelli +9
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Pulsars and Gravitational Waves Research #gr-qc
paper · pdf · doi:10.48550/arxiv.gr-qc/0012110
2 pages, contribution to the 9th Marcel Grossmann meeting (MG9), Rome, July 2000
arxiv created 2000/12/29 · openalex publication_date 2000/12/29 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We present a characteristic algorithm for computing the perturbations of a Schwarzschild spacetime by means of solving the Teukolsky equations. Our methods and results are expected to have direct bearing on the study of binary black holes presently underway using a fully \em nonlinear characteristic code \citeGomez98a.