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山田研究室
Showing the original Japanese · View translation
超新星やブラックホールの謎を理論で解き明かす研究室。
AboutAbout the lab
星の最期に迫る、理論宇宙物理学。
山田研究室は、
太陽よりはるかに
その
ガンマ線バーストや、
Key terms
- 重力崩壊
- 星が
自らの 重さを 支えられなくなり、 中心部が 急激に つぶれる 現象 - 中性子星
- 星が
重力崩壊した あとに できる、 非常に 密度の 高い天体 - マグネター
- 非常に
強い 磁場を 持つ、 特殊な 中性子星
NewsLab news
View More ↗ResearchResearch themes
太陽よりはるかに
*Illustrative image超新星爆発と中性子星の形成
とても
*Illustrative imageブラックホール形成の理論
重力崩壊で
*Illustrative imageガンマ線バーストと連星系
ブラックホール形成には
*Illustrative imageマグネターの物理
非常に
MembersFaculty
山田研究室の
- Professor山田 章一
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RelatedLabs similar to 山田研究室
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: “Keplers supernova” NASA/ESA/JHU/R.Sankrit & W.Blair / Public domain (cropped)
- 超新星爆発と
中性子星の 形成: “Red onion cross section 04” Amada44 / CC BY-SA 3.0 (cropped) - ブラックホール形成の
理論: “Illustration of an Isolated Black Hole ( )” NASA Hubble / Public domain (cropped) - ガンマ線バーストと
連星系: “Artist’s impression of a gamma-ray burst shining through two young galaxies in the early Universe” ESO/L. Calçada / CC BY 4.0 (cropped) - マグネターの
物理: “Artist’s impression of the magnetar in the star cluster Westerlund 1” ESO/L. Calçada / CC BY 4.0 (cropped) - Related lab (辻川研究室): “Illustris Dark Matter and Gas” Illustris Collaboration / CC BY-SA 4.0 (cropped)
- Related lab (井上研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
- Related lab (鷹野研究室): “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped)
- Related lab (高野研究室): “Crowded cytosol” TimVickers / Public domain (cropped)
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