| 日時: |
2008-07-22 11:00 - 12:00 |
| 場所: |
研究本館２階２２０室 |
| 会議名: |
Astrophysical Accelerators and High-Energy Neutrino Astronomy (in English) |
| 連絡先: |
津田 |
| 講演者: |
村瀬 孔大 氏 (京都大学基礎物理学研究所) |
| 講演言語: |
英語 |
| アブストラクト: |
The origin of high-energy cosmic rays is one of the big mysteries in the Universe. Detection of high-energy neutrinos and gamma rays will be useful as a probe of cosmic-ray acceleration in astrophysical sources. Now, large neutrino telescopes such IceCube and KM3Net are being constructed, and not only high-energy gamma-ray astronomy but also neutrino astronomy may be possible in the future. In my talk, we will discuss possibilities of high-energy cosmic-ray acceleration in extragalactic objects such as gamma-ray bursts, active galactic nuclei and clusters of galaxies. The high-energy neutrino emission from such objects and future prospects will mainly be discussed.
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