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高田昌広研究室
Showing the original Japanese · View translation
すばる望遠鏡の銀河サーベイで、暗黒物質と暗黒エネルギーに迫る研究室。
AboutAbout the lab
宇宙の構造から、見えないものを測る。
高田研究室は、
宇宙の
暗黒エネルギーや
すばる
Key terms
- 暗黒エネルギー
- 宇宙の
膨張を 加速させていると 考えられている、 正体 不明の エネルギー - 重力レンズ効果
- 重い天体の
重力で 光の 進む道が 曲がり、 その 奥の 天体の 像が ゆがんで 見える 現象 - 銀河サーベイ
- 望遠鏡で
広い 空の 範囲を くまなく 撮り、 たくさんの 銀河の 位置や形を 調べる 観測
ResearchResearch themes
カブリ数物連携宇宙研究機構が
*Illustrative image重力レンズで探る暗黒物質と暗黒エネルギー
宇宙の
*Illustrative image銀河の分布からニュートリノの質量を制限
銀河が
*Illustrative image重力理論と構造形成モデルの検証
宇宙論の
MembersFaculty
- Professor高田 昌広
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: “Subaru mk summit light” Avriette at en.wikipedia / CC BY-SA 3.0 (cropped)
- 重力レンズで
探る 暗黒物質と 暗黒エネルギー: “Gravitational lensing in the galaxy cluster Abell 370 (captured by the Hubble Space Telescope)” NASA, ESA, the Hubble SM4 ERO Team and ST-ECF / CC BY 4.0 (cropped) - 銀河の
分布から ニュートリノの 質量を 制限: “Hubble ultra deep field” NASA and the European Space Agency / Public domain (cropped) - 重力理論と
構造形成モデルの 検証: “Cosmic web” Volker Springel / Max Planck Institute For Astrophysics / CC BY-SA 4.0 (cropped)
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