Abstract
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.
| Original language | English |
|---|---|
| Title of host publication | Proceedings of the 15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005 |
| Pages | 175-178 |
| Number of pages | 4 |
| Publication status | Published - Dec 1 2005 |
| Event | 15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005 - Tokyo, Japan Duration: Nov 28 2005 → Dec 2 2005 |
Other
| Other | 15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005 |
|---|---|
| Country | Japan |
| City | Tokyo |
| Period | 11/28/05 → 12/2/05 |
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All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
Cite this
Gravitational wave from realistic stellar collapse : Odd parity perturbation. / Kiuchi, Kenta; Nakazato, Ken'ichiro; Kotake, Kei; Sumiyoshi, Kohsuke; Yamada, Shoichi.
Proceedings of the 15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005. 2005. p. 175-178.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - Gravitational wave from realistic stellar collapse
T2 - Odd parity perturbation
AU - Kiuchi, Kenta
AU - Nakazato, Ken'ichiro
AU - Kotake, Kei
AU - Sumiyoshi, Kohsuke
AU - Yamada, Shoichi
PY - 2005/12/1
Y1 - 2005/12/1
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=84887438615&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84887438615&partnerID=8YFLogxK
M3 - Conference contribution
AN - SCOPUS:84887438615
SP - 175
EP - 178
BT - Proceedings of the 15th Workshop on General Relativity and Gravitation in Japan, JGRG 2005
ER -