Resonance between Primordial Gravitational Waves and a Galaxy
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概要
- 論文の詳細を見る
We present numerical simulations of a tidal deformation of a galaxy due to an interaction with intense primordial gravitational waves of wavelength of typically 30 Mpc. The galaxy is found to be deformed to a trailing spiral shape within one revolution time. In contrast to Toomre and Toomre's simulation of colliding galaxies, the present deformation of a galaxy is bi-symmetric about its rotational axes. The deformation in the direction perpendicular to the galactic plane is found to be negligible for any incident angle of the gravitational wave.
- 理論物理学刊行会の論文
- 1979-05-25
著者
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FUTAMASE Toshifumi
Department of Astronomy, Graduate School of Science, Tohoku University
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Futamase Toshifumi
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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MATSUDA Tastuya
Department of aeronautical Engineering, Faculty of Engineering Kyoto University
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Matsuda Tastuya
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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Matsuda Takuya
Department Of Aeronautical Engineering Faculty Of Engineering Kyoto University
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FUTAMASE Toshifumi
Department of aeronautical Engineering, Faculty of Engineering Kyoto University
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