期刊
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
卷 47, 期 3, 页码 765-771出版社
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-007-9500-5
关键词
quasinormal modes; Schwarzschild black hole; Ricci tensor
We recalculate the Ricci tensors of non-stationary axisymmetric space-times originally calculated by Chandrasekhar, and we find that in the linear regime there are some common factors that did not appear in the original results. We also find some discrepancies in the non-linear terms. However, these discrepancies do not affect the well-known results concerning linear perturbations of a Schwarzschild black hole.
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