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Hellerman研究室(Kavli IPMU)
Showing the original Japanese · View translation
ストリング理論で、時空のごく短い距離での重力の姿を探る研究室。
AboutAbout the lab
ストリング理論で、重力と宇宙を解く。
Hellerman研究室は、
初期宇宙のように、
ストリング理論は、
ストリング理論の
Key terms
- ストリング理論
- 素粒子を
点ではなく、 広がりを もつ弦（ストリング）と して 考える 理論。 重力も 含めて 扱える - 不確定性原理
- 粒子の
位置と 運動量のように、 組に なる量を 同時に 正確には 決められないと いう 量子力学の 原理 - 超対称性
- 物質を
つくる 粒子と、 力を 伝える 粒子とを 入れ替える 対称性
ResearchResearch themes
時空の
*Illustrative image短い距離での重力のダイナミクス
初期宇宙のように、
*Illustrative imageストリング理論の相と相転移
宇宙論的な
MembersFaculty
- ProfessorSimeon John Hellerman
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: “CY5-6D-lattice” Andrew J. Hanson / CC BY-SA 3.0 (cropped)
- 短い
距離での 重力の ダイナミクス: “Worldsheet” Anna.g / CC BY-SA 3.0 (cropped) - ストリング理論の
相と 相転移: “CalabiYau5” Andrew J. Hanson / CC BY-SA 3.0 (cropped)
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