Gravitational Quasinormal Modes of Regular Phantom Black Hole

We investigate the gravitational quasinormal modes (QNMs) for a type of regular black hole (BH) known as phantom BH, which is a static self-gravitating solution of a minimally coupled phantom scalar field with a potential. The studies are carried out for three different spacetimes: asymptotically fl...

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Bibliographic Details
Main Authors: Jin Li, Kai Lin, Hao Wen, Wei-Liang Qian
Format: Article
Language:English
Published: Hindawi Limited 2017-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2017/5234214