Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence

Details Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence

2006-11-28

arxiv.org/abs/gr-qc/0611146v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, 2 figures

Scientific paper

We present the quasinormal frequencies of the massive scalar field in the background of a Schwarzchild black hole surrounded by quintessence with the third-order WKB method. The mass of the scalar field $u$ plays an important role in studying the quasinormal frequencies, the real part of the frequencies increases linearly as mass $u$ increases, while the imaginary part in absolute value decreases linearly which leads to damping more slowly and the frequencies having a limited value. Moreover, owing to the presence of the quintessence, the massive scalar field damps more slowly.

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