Massive scalar field quasinormal modes of a black hole in the deformed Hořava-Lifshitz gravity

• Authors: ChunYan Wang , YaJun Gao
• Languages of publication: EN

Abstracts

EN

We calculated the quasinormalmodes ofmassive scalar field of a black hole in the deformed Hořava-Lifshitz gravity with coupling constant λ = 1, using the third-order WKB approximation. Our results show that when the scalar field mass increases, the oscillation frequency increases while the damping decreases. And we find that the imaginary parts are almost linearly related to the real parts, the behaviors are very similar to that in the Reissner-Nordström black hole spacetime. These information will help us understand more about the Hořava-Lifshitz gravity.

Keywords

EN

Hořava-Lifshitz gravity; quasinormal frequencies; WKB approximation

• Publisher: De Gruyter Open
• Journal: Open Physics
• Year: 2012
• Volume: 10
• Issue: 1
• Pages: 40-46

Dates

published

1 - 2 - 2012

online

3 - 12 - 2011

Contributors

author

ChunYan Wang

• Department of Physics, School of Mathematics and Physics, Bohai University, Jinzhou, 121013, P. R. China

author

YaJun Gao

• Department of Physics, School of Mathematics and Physics, Bohai University, Jinzhou, 121013, P. R. China

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Identifiers

DOI

10.2478/s11534-011-0097-1