首页 | 本学科首页   官方微博 | 高级检索  
     检索      


Quasinormal Modes of Spherically Symmetric Curve Spacetime with Dark Matter Term
Authors:Yan Zhang  Ying Zhou  Guo-Ping Li
Institution:1. Institute of Theoretical Physics, China West Normal University, Nanchong, 637002, China
2. School of Physical Electronics, University of Electronic Science and Technology of China, Chengdu, 610054, China
Abstract:We study quasinormal modes of scalar field perturbation and electromagnetic field perturbation in a black hole space-time with dark matter by using WKB approximation method. The result shows clearly that the real part of black hole quasinormal modes is mainly determined by angular quantum number while its imaginary part mainly determined by model number. We also found out that the dark matter will restrain the perturbation frequency and slow down the speed of damping in spacetime. In addition; dark matter has a greater influence upon quasinormal modes in the electromagnetic field than that in the scalar field.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号