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

• Autorzy: Chunrui Ma , Yuanxing Gui , Wei Wang , Fujun Wang
• Języki publikacji: EN

Abstrakty

EN

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 of the field u increases, while the imaginary part in absolute value decreases linearly which leads to damping more slowly than the massless scalar field. The frequencies have a limited value, so it is easier to detect the quasinormal modes. Moreover, owing to the presence of the quintessence, the massive scalar field damps more slowly.

Słowa kluczowe

EN

black hole; quasinormal; quintessence

• Czasopismo: Open Physics
• Rocznik: 2008
• Tom: 6
• Numer: 2
• Strony: 194-198

Daty

wydano

2008-06-01

online

2008-03-26

Twórcy

autor

Chunrui Ma

• School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China,

autor

Yuanxing Gui

• School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China

autor

Wei Wang

• College of Physical Science and Technology of Dalian University, 116024, Dalian, China

autor

Fujun Wang

• School of Physics and Optoelectronic Technology, Dalian university of Technology, 116024, Dalian, China

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Identyfikatory

DOI

10.2478/s11534-008-0056-7