期刊
INTERNATIONAL JOURNAL OF MODERN PHYSICS D
卷 14, 期 3-4, 页码 543-571出版社
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S021827180500592X
关键词
Newton stars; gravitational waves; general relativity
We present a hyperbolic formulation of the evolution equations describing nonradial perturbations of slowly rotating relativistic stars in the Regge-Wheeler gauge. We demonstrate the stability properties of the new evolution set of equations and compute the polar w-modes for slowly rotating stars.
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