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电磁扰动下Kerr-Newman黑洞的拟正则模

The quasinormal modes of Kerr-Newman black hole
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摘要 对黑洞周围场的拟正则模的研究有助于证实黑洞的存在和揭示其内部性质.选取Kerr-Newman黑洞作为研究对象,以电磁场作为初始扰动场,运用数值模拟方法给出若干客观的图像,并分析、讨论黑洞的不同参量对拟正则模的影响. The study on the quasinormal modes of field around black holes will be helpful to testify the existence and reveal the nature of black holes. In this paper, we take the Kerr-Newman black holes as study object and electromagnetic field as an initial perturbation field. After presenting some object pictures from numerical simulation, we analyze and discuss the different effects caused by different parameters of black holes.
出处 《上海师范大学学报(自然科学版)》 2008年第2期148-152,共5页 Journal of Shanghai Normal University(Natural Sciences)
基金 上海市科委项目(04dz05905)
关键词 Kerr—Newman黑洞 电磁场 拟正则模 数值模拟 Kerr-Newman black holes electromagnetic field quasinormal modes numerical simulation
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参考文献10

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