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鷹野研究室
Showing the original Japanese · View translation
原子核の理論から、中性子星や超新星爆発にせまる研究室。
AboutAbout the lab
原子核の理論で、星の中をのぞく。
鷹野研究室は、
原子核は
そこで、
得られた
Key terms
- 核物質
- 無限個の
核子から できた、 無限に 大きい 仮想的な 原子核。 原子核の 大局的な 性質を 調べる ために 考える - 状態方程式
- 物質の
エネルギーや 圧力が、 密度などと どう 関係するかを 表す式 - 変分法
- 厳密に
解けない 問題で、 答えの 形を あらかじめ仮定し、 もっとも 良い ものを 選び出す計算の やり方
ResearchResearch themes
原子核の
*Illustrative image核物質の状態方程式
鉛の
*Illustrative image中性子星と超新星爆発への応用
中性子星は
*Illustrative image量子多体系と原子核質量の研究
核物質と
MembersFaculty
鷹野研究室の
- Professor鷹野 正利
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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: “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped)
- 核物質の
状態方程式: “Dutch national supercomputer "Huygens"” Dennis van Zuijlekom / CC BY-SA 2.0 (cropped) - 中性子星と
超新星爆発への 応用: “Neutron Star Illustration ( -more-1)” CXC/M. Weiss / Public domain (cropped) - 量子多体系と
原子核質量の 研究: “Liquid helium superfluid phase” Alfred Leitner （アップロード：Bmatulis） / Public domain (cropped) - Related lab (山田研究室): “Keplers supernova” NASA/ESA/JHU/R.Sankrit & W.Blair / Public domain (cropped)
- Related lab (辻川研究室): “Illustris Dark Matter and Gas” Illustris Collaboration / CC BY-SA 4.0 (cropped)
- Related lab (高野研究室): “Crowded cytosol” TimVickers / Public domain (cropped)
- Related lab (上田研究室): “Osteosarcoma cells stained for actin, microtubules, and nuclei” Howard Vindin / CC BY 4.0 (cropped)
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