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竹田敦研究室(ICRR宇宙ニュートリノ研究部門)
Showing the original Japanese · View translation
ニュートリノと暗黒物質から、宇宙の誕生と進化を解き明かす研究室。
AboutAbout the lab
ミクロの粒子で、宇宙の歴史を解く。
竹田研究室は、
ニュートリノは
スーパーカミオカンデを
イタリアで
Key terms
- ニュートリノ
- 電気を
帯びず、 ほかの 物質と ほとんど 反応しない 素粒子。 星の 内部や 超新星爆発で 大量に 生まれる - 暗黒物質
- 光では
見えないが、 重力の 効果から 宇宙に 大量に あると 考えられている 正体 不明の 物質 - 水チェレンコフ検出器
- 大量の
水の 中を 荷電粒子が 走る ときに 出る 青白い 光 （チェレンコフ光）を とらえて 粒子を 観測する 装置
ResearchResearch themes
宇宙が
*Illustrative imageニュートリノで探る物質と宇宙の進化
宇宙が
*Illustrative imageハイパーカミオカンデの建設
スーパーカミオカンデを
*Illustrative image暗黒物質の直接検出と超新星ニュートリノ
イタリアで
MembersFaculty
- Associate Professor竹田 敦Publications ↗
VoicesStudent voices
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Hyper-Kamiokande under constracting 02” 文部科学省 / CC BY 4.0 (cropped)
- ニュートリノで
探る 物質と 宇宙の 進化: “HK experiment overview” Jan Kisiel (Silesia U.) for the Hyper-Kamiokande collaboration / CC BY 4.0 (cropped) - ハイパーカミオカンデの
建設: “Hyper-Kamiokande scheme” Shota Izumiyama (Tokyo Inst. Tech.) for the Hyper-Kamiokande collaboration / CC BY 3.0 (cropped) - 暗黒物質の
直接検出と 超新星ニュートリノ: “Solid and liquid xenon” Solypewo / CC BY-SA 4.0 (cropped)
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