MG14 - Talk detail |
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Participant |
Shibata, Masaru | |||||||
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Institution |
Yukawa Institute for Theoretical Physics, Kyoto University - Kitashirakawa, Oiwakecho, Sakyo-ku - Kyoto - Kyoto - Japan | |||||||
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Session |
BN2 |
Accepted |
Yes |
Order |
6 |
Time |
15:45 | 15' |
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Talk |
Oral abstract |
Title |
Merger of binary neutron stars: Latest progress in Kyoto | |||||
| Coauthors | Kiuchi, Kenta; Sekiguchi, Yu-ichiro; Kyutoku, Koutarou | |||||||
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Abstract |
The merger of binary neutron stars is among the most promising gravitational wave sources for km-size laser-interferometers, a plausible candidate for short-hard gamma-ray bursts, and possible site for r-process nucleosynthesis. To explore these aspects of the merger, numerical-relativity simulations are required. We have been performing a wide variety of numerical-relativity simulations including magnetohydrodynamics simulations and neutrino-radiation transfer simulations. I will report our latest activities for these simulations. |
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Pdf file |
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