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Kavli IPMU CMB Group(松村研究室)
Showing the original Japanese · View translation
宇宙最古の光の偏光から、宇宙の始まりに迫る研究室。

AboutAbout the lab
宇宙の始まりを、CMBの偏光で確かめる。
松村研究室
宇宙の
この
国際共同研究が
Key terms
- 宇宙マイクロ波背景放射
- 宇宙が
生まれて間も ない ころの 光が、 宇宙の 膨張で 波長が 伸び、 電波と して 全天から 届いている もの - インフレーション
- 宇宙が
生まれた 直後の ごく 短い 時間に、 空間が 急激に 膨張したとする 考え - 偏光
- 光の
波が 振動する 向きのかたより
ResearchResearch themes
インフレーション仮説を
*Illustrative imageCMB偏光観測衛星LiteBIRD
JAXA宇宙科学研究所の
*Illustrative image地上望遠鏡 Simons Observatory
Simons Observatory は、
*Illustrative imageミリ波・テラヘルツの光学素子
レンズ、
*Illustrative image極低温で動く機構の開発
液体窒素や
MembersFaculty
松村研究室の
- Associate Professor松村 知岳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. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “LAT SO” Flucerod / CC BY-SA 4.0 (cropped)
- CMB偏光観測衛星LiteBIRD: “LiteBIRD CG03” JAXA
(ISAS ギャラリー https://isas-gallery.jp/3853) / CC BY 4.0 (cropped) - 地上望遠鏡 Simons Observatory: “SO SAT render” Sdicker / CC BY-SA 4.0 (cropped)
- ミリ波・テラヘルツの
光学素子: “Optical-waveplate-1inch” Geek3 / CC BY-SA 4.0 (cropped) - 極低温で
動く 機構の 開発: “Magnetic levitation of a superconductor” Your stepbro sunset / CC BY 4.0 (cropped)
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