High Frequency Gravitational Radiation and Ringing Down of an Isolated Gravitating System
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概要
- 論文の詳細を見る
A qualitative description is given of the gravitational field of an isolated gravitating system emitting high frequency gravitational radiation which is ended by a burst of radiation accompanied by matter travelling with the speed of light, which in turn is followed by an exponential ringing down to the field of a spherical black hole.The process we describe could conceivably be applied to the last stages of a binary neutron star collision.In this case the high frequency phase coincides with the rapid inspiral motion of the stars.This is ended by the collision, giving rise to a burst of outgoing radiation accompanied by light-1ike matter such as neutrinos, and then the ringing down follows when the remnant of the collision rapidly radiates away its wave-front anisotropy, and a spherical black hole is formed.
- 理論物理学刊行会の論文
- 2000-06-25
著者
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FUTAMASE Toshifumi
Astronomical Institute, Tohoku University
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Futamase Toshifumi
Department Of Physics Hirosaki University
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Futamase Toshifumi
Astronomical Institute Graduate School Of Science Tohoku University
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HOGAN Peter
Mathematical Physics Department University College Dublin
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FUTAMASE Toshifumi
Astronomical Institute Graduate School of Science, Tohoku University
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