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鈴木研究室
Showing the original Japanese · View translation
超新星爆発の物理を理論から探る研究室。
AboutAbout the lab
超新星の物理を、理論で探る。
鈴木研究室は、
研究室の
プロジェクトには、
も
Key terms
- 超新星
- 星が
一生の 最後に 起こす 大きな 爆発現象。 爆発の ときに ニュートリノが 放出される - 中性子星
- 超新星爆発の
あとに 残る、 極めて 高密度な天体 - 状態方程式
- 物質の
密度や 圧力などの 関係を 表す式。 研究室の サイトに 中性子星物質の 状態方 程式が 載っている
ResearchResearch themes
この
MembersFaculty
- Professor鈴木 英之
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: “Neutron Star X-ray beaming with accretion disk” NASA / Public domain (cropped)
- Related lab (澤渡研究室): “Neel skyrmion models” Börge Göbel, Ingrid Mertig, Oleg A.Tretiakov / CC BY 4.0 (cropped)
- Related lab (石塚研究室): “CHIPS-M neutrino detector ( )” UCL Mathematical and Physical Sciences from London, UK / CC BY 2.0 (cropped)
- Related lab (阿部研究室): “Zeus jul08” Luis Sanchez (talk) / CC BY-SA 3.0 (cropped)
- Related lab (吉岡研究室): “Morpho peleides Niagara Parks Butterfly Conservatory” The Cosmonaut / CC BY-SA 2.5 ca (cropped)
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