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松本重貴 研究グループ(Kavli IPMU)
Showing the original Japanese · View translation
素粒子物理学の立場から、暗黒物質の正体に迫る研究室。
AboutAbout the lab
暗黒物質の正体から、新しい物理へ。
松本研究室は、
暗黒物質は
まず
研究の
Key terms
- 暗黒物質
- 光では
見えず、 重力を 通してだけ存在が 分かる 正体 不明の 物質 - 標準模型
- これまでに
見つかった 素粒子と、 その間に 働く 力を まとめた 理論 - WIMP
- ほかの
粒子と ごく 弱くしか 反応しない 重い 未知の 粒子。 暗黒物質の 有力な 候補と される
ResearchResearch themes
暗黒物質の
MembersFaculty
- Professor松本 重貴Publications ↗
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.
- Top image: “Hubble maps dark matter web in a large galaxy cluster (heic0802b)” Credit for the Hubble images: NASA, ESA, C. Heymans (University of British Columbia, Vancouver), M. Gray (University of Nottingham, U.K.), M. Barden (Innsbruck), and the STAGES collaboration Credit for the ground-based image: ESO, C. Wolf (Oxford University, U.K.), K. Meisenheimer (Max-Planck Institute for Astronomy, Heidelberg), and the COMBO-17 collaboration / Public domain (cropped)
- 素粒子物理学から
迫る 暗黒物質: “Large Underground Xenon detector inside watertank” Gigaparsec (English Wikipedia) / CC BY 3.0 (cropped)
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