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中村研究室
Showing the original Japanese · View translation
不安定な原子核の実験から、物質と宇宙の謎を探る研究室。
AboutAbout the lab
不安定な原子核から、物質と宇宙の謎へ。
中村研究室は、
特に
実験は
研究室は、
Key terms
- 不安定核
- 天然には
存在せず、 すぐに 壊れてしまう 寿命の 短い 原子核。 加速器を 使って つくる - 中性子ハロー核
- 中心の
芯の まわりを、 中性子が 薄く 広く 取り巻いている 原子核 - 魔法数
- 陽子や
中性子が この 数だけ集まると、 原子核が 特に 安定に なると いう 特別な 数 - 状態方程式
- 物質の
圧力や エネルギーが、 密度に よって どう 変わるかを 表す関係
ResearchResearch themes
天然には
*Illustrative image中性子ハロー核
中
*Illustrative image原子核の殻構造の変化
原子核は、
*Illustrative image天体核反応
鉄より
*Illustrative image中性子星の核物質
中性子星の
MembersFaculty
中村研究室の
- Professor中村 隆司Publications ↗
- Project Associate Professor佐藤 義輝
- Assistant Professor花井 周太郎
VoicesStudent voices
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The information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
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 P4213478” Kestrel / CC BY-SA 4.0 (cropped)
- 中性子ハロー核: “RIKEN BigRIPS P4213487” Kestrel / CC BY-SA 4.0 (cropped)
- 原子核の
殻構造の 変化: “Nuclear Physicists Wield HPC to Uncover Magic Isotopes” OLCF / CC BY 2.0 (cropped) - 天体核反応: “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped)
- 中性子星の
核物質: “Neutron Star X-ray beaming with accretion disk” NASA / Public domain (cropped) - Related lab (高峰研究室): “NuclideMap stitched 2” NuclideMap.PNG: The viewer derivative work: Neokortex (talk) / Public domain (cropped)
- Related lab (関澤研究室): “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped)
- Related lab (藤岡研究室): “J-PARC Hadron Experimental Facility 1” Kestrel / CC BY-SA 4.0 (cropped)
- Related lab (慈道研究室): “Quantum Fluctuations” Derek Leinweber / CC BY-SA 4.0 (cropped)
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