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- W2109407129 abstract "We study the evolution of massive scalar field in the spacetime geometry of Kehagias-Sfetsos black hole in deformed Hořava-Lifshitz (HL) gravity by numerical analysis. We find that the signature of HL theory is encoded in the quasinormal mode (QNM) phase of the evolution of field. The QNM phase in the evolution process lasts for a longer time in HL theory. QNMs involved in the evolution of massive field are calculated and find that they have a higher oscillation frequency and a lower damping rate than the Schwarzschild spacetime case. We also study the relaxation of field in the intermediate and asymptotic range and verified that behaviors of field in these phases are independent of the HL parameter and is identical to the Schwarzschild case." @default.
- W2109407129 created "2016-06-24" @default.
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- W2109407129 date "2011-06-04" @default.
- W2109407129 modified "2023-09-24" @default.
- W2109407129 title "Evolution of massive fields around a black hole in Hořava gravity" @default.
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- W2109407129 doi "https://doi.org/10.1007/s10714-011-1201-y" @default.
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