We study gravitational wave from massive stellar core collapse with the spherical symmetry. We choose a perfect Huid with the realistic equation of state as a matter. The gauge-invariant approach is adopted to estimate the gravitational wave. Performing the numerical simulation, the waveform and the frequency for I = 2 are obtained. Analyzing the result of the simulation, we find that the gravitaional wave is produced at the core bounce. The frequency is about 1Hz.
|出版ステータス||Published - 2005 12月 1|
|イベント||15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005 - Tokyo, Japan|
継続期間: 2005 11月 28 → 2005 12月 2
|Conference||15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005|
|Period||05/11/28 → 05/12/2|
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