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〈素粒子物理学〉
Showing the original Japanese · View translation
素粒子物理の理論で暗黒物質やニュートリノを探る研究。
AboutAbout the lab
暗黒物質を、理論から探る。
藤原素子准教授は、
中性子星の
高校生への
共創学部の
Key terms
- ディグリープロジェクト
- 共創学部の
卒業研究に あたる 科目。 成果は 論文の ほか、 制作物、 政策提言、 社会実践でも よい - スパイク
- 超巨大ブラックホールの
近くで、 暗黒物質の 密度が 極めて 高くなった 領域 - 潮汐破壊現象
- ブラックホールの
近くを 通った 星が、 強い 重力で 引き裂かれる 現象
ResearchResearch themes
素粒子の
*Illustrative image中性子星で探る暗黒物質
中性子星の
*Illustrative image暗黒物質のガンマ線シグナル
暗黒物質の
*Illustrative image暗黒物質スパイクとニュートリノ
共同研究と
*Illustrative image宇宙初期の磁場の進化
共同研究と
MembersFaculty
- Associate Professor藤原 素子
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: “Webb Data Reveals Dark Matter (PIA26702)” NASA Jet Propulsion Laboratory / NASA/STScI/J. DePasquale/A. Pagan / Public domain (cropped)
- 中性子星で
探る 暗黒物質: “Degenerate star sizes” Grufo / CC0 (cropped) - 暗黒物質の
ガンマ線シグナル: “Fermi Gamma-ray Space Telescope spacecraft model” NASA / Public domain (cropped) - 暗黒物質スパイクと
ニュートリノ: “Black hole - Messier 87 crop max res” Event Horizon Telescope, uploader cropped and converted TIF to JPG / CC BY 4.0 (cropped) - 宇宙初期の
磁場の 進化: “Peering Back to the Early Universe (peering-back-to-the-early-universe-1)” Image: NASA, ESA, CSA, S. Finkelstein (UT Austin), M. Bagley (UT Austin), R. Larson (UT Austin). Image processing: A. Pagan (STScI) / CC BY 4.0 (cropped) - Related lab (地球物理学
（大野 正夫） ): “Tavurvur volcano edit” Taro Taylor edit by Richard Bartz / CC BY 2.0 (cropped) - Related lab (〈海洋物理学〉): “Pacific-garbage-patch-map 2010 noaamdp” NOAA / Public domain (cropped)
- Related lab (海洋物理学
（木田 新一郎） ): “Sediment in the Bohai Sea, Yellow Sea, and East China Sea (MODIS )” MODIS Land Rapid Response Team, NASA GSFC / Public domain (cropped) - Related lab (〈自然地理学〉): “Malolo Barrier Reef 5” Maksym Kozlenko / CC BY-SA 4.0 (cropped)
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