Dirac Quasinormal Modes of Static f(R) de Sitter Black Holes

• 来源期刊: 理论物理通讯（英文版）
• 年，卷（期）: 2018,（2）
• 页码范围: 179-187
• 页数: 9页
• 语种: 英文
• DOI: 10.1088/0253-6102/69/2/179

摘要

Quasinormal modes (QNMs) for Dirac perturbations of f(R) black holes (BHs) are described in this paper,involving two types of f(R) solution:f(R) (Schwarzschild) BHs and f(R) (Maxwell) BHs.With the finite difference method,the stability of the f(R) black holes (BHs) is analysed and the threshold range off(R) (Schwarzschild) BHs and f(R) (Maxwell) BHs is defined respectively.The results show that due to the presence of the correction factor Ro,the damping rate of Dirac field decreases.Meanwhile,the influence of angular quantum number values [k[on the f (R) BHs is investigated.The results indicate that the QNMs oscillation becomes tenser and damping speed slowly decreases with [k[increasing.Furthermore,under the Dirac perturbation,the stability of f (R) solutions can be reflected in the manner of Dirac QNMs.The relationships between the QNMs and the parameters ([k|,charge Q and mass m) are discussed in massless,and massive cases,by contrast to the classical BHs.