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Object Picture of Electromagnetic Quasinormal Ringing for a Stringy Black Hole

Object Picture of Electromagnetic Quasinormal Ringing for a Stringy Black Hole
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摘要 We investigate the evolution of an electromagnetic field in the spacetime of a stringy black hole.The objectpicture of the quasinormal ringing has been obtained by the finite difference method.Compared with a Schwarzschildblack hole,the results show that the electromagnetic field damps more slowly for a stringy black hole.
出处 《Communications in Theoretical Physics》 SCIE CAS CSCD 2008年第12期1345-1347,共3页 理论物理通讯(英文版)
基金 National Natural Science Foundation of China under Grant No.10573004
关键词 Iquasinormal modes quasinormal ringing finite difference method 黑洞 场扰动 演化 时空背景 理论物理学
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