Abstract The late-time tails of massless and self-interacting (SI) (massive) scalar fields are investigated analytically in a stationary axisymmetric Einstein—Maxwell dilaton-axion (EMDA) black hole geometry. It is shown that the asymptotic behaviour of massless perturbations is dominated by an inverse power-law decaying tail and the intermediate asymptotic behaviour of SI (massive) perturbations is dominated by an oscillatory one.
Received: 20 May 2004
Revised: 14 July 2004
Accepted manuscript online:
Fund: Project supported by the National Natural Science Foundation of China (Grant No 10275024); the FANEDD (Grant No 200317); and the Hunan Provincial Natural Science Foundation of China (Grant No 04JJ3019).
Cite this article:
Pan Qi-Yuan (潘启沅), Jing Ji-Liang (荆继良) Late-time tails in a stationary axisymmetric EMDA black hole geometry 2005 Chinese Physics 14 268
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