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鈴木研究室
Showing the original Japanese · View translation
RIビームで原子核と核物質のなぞに挑む、原子核実験の研究室。
AboutAbout the lab
原子核から、中性子星の中身まで。
鈴木研究室は、
放射性同位体
主な
2024年12月に
Key terms
- 放射性同位体
- 陽子と
中性子の 数が 偏っていて、 放射線を 出して 別の 原子核に 変わる 不安定な 原子核。 RIとも 呼ぶ - 開放量子系
- 原子核の
中で 結合が 「ゆる い」状態。 すぐに 粒子が こぼれ出てしまう ため、 調べるのが とても 難しい - 中性子星
- 重い星が
超新星爆発を 起こした あとに 残る、 主に 中性子から なるとても 密度の 高い 星
NewsLab news
View More ↗ResearchResearch themes
陽子・中性子・パイ中間子から
*Illustrative image核構造の創発現象とガンマ線核分光
原子核の
*Illustrative image原子核に現れる開放量子系
結合が
*Illustrative imageRIと宇宙元素合成・中性子星
宇宙の
MembersFaculty
鈴木研究室の
- Associate Professor鈴木 大介
- Assistant Professor北村 徳隆Publications ↗
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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: “RIKEN Superconducting Ring Cyclotron P4208172” Kestrel / CC BY-SA 4.0 (cropped)
- 核構造の
創発現象と ガンマ線核分光: “Frosted cryostat of a High-Purity Germanium (HPGe) detector” Bibric02 / CC0 (cropped) - 原子核に
現れる 開放量子系: “RIKEN BigRIPS P4208204” Kestrel / CC BY-SA 4.0 (cropped) - RIと
宇宙元素合成・中性子星: “Neutron Star Merger (noirlab2518f)” International Gemini Observatory/NOIRLab/NSF/AURA/Double Dome Films / CC BY 4.0 (cropped) - Related lab (中村研究室): “Artist's Illustration of Neutron Star (2009-cassio-more-2 - neutron)” X-ray: NASA/CXC/Southampton/W. Ho et al.; Illustration: NASA/CXC/M.Weiss / Public domain (cropped)
- Related lab (福嶋研究室): “Lead-Ion Collision at NA49-CERN” CERN PhotoLab / CC BY 4.0 (cropped)
- Related lab (Liang研究室): “NuclideMap stitched 2” NuclideMap.PNG: The viewer derivative work: Neokortex (talk) / Public domain (cropped)
- Related lab (矢向研究室
（CNS実験核物理） ): “RIKEN Superconducting Ring Cyclotron P4213478” Kestrel / CC BY-SA 4.0 (cropped)
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