Asymptotic quasinormal modes of scalar field in a gravity's rainbow

• 来源期刊: 中国物理B（英文版）
• 关键词: gravity's rainbow quasinormal modes monodromy method quantum effect
• 年，卷（期）: 2009,（10）
• 页码范围: 4161-4168
• 页数: 8页
• 语种: 英文

摘要

In the framework of the gravity's rainbow, the asymptotic quasinormal modes of the modified Schwarzschild black holes undergoing a scalar perturbation are investigated. By using the monodromy method, we analytically calculated the asymptotic quasinormal frequencies, which depend on not only the mass parameter of the black hole, but also the particle's energy of the perturbation field. Meanwhile, the real parts of the asymptotic quasinormal modes can be expressed as TH ln3, which is consistent with Hod's conjecture. In addition, for the quantum corrected black hole, the area spacing is independent of the particle's energy, even though the area itself depends on the particle's energy. And that, by relating the area spectrum to loop quantum gravity, the Barbero-Immirzi parameter is given and it remains the same as from the usual black hole.