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仏坂研究室
Showing the original Japanese · View translation
中性子星やブラックホールの合体を、重力波と光で読み解く、宇宙物理理論の研究室。
AboutAbout the lab
重力波と光で、星の合体を読み解く。
仏坂研究室は、
中心に
主に
Key terms
- 重力波
- 重い天体が
激しく 動いた ときに、 時空の ゆが みが 波と なって光の 速さで 伝わる 現象 - 中性子星
- 重い星が
一生の 最後に 爆発した あとに 残る、 ほとんど 中性子で できた とても 密度の 高い 星 - 数値相対論
- アインシュタインの
一般相対性理論の 式を、 コンピュータで 数値的に 解いて天体の 動きを 調べる 方法 - キロノバ
- 中性子星の合体で
飛び出した 物質の 中で 重い 元素が 作られ、 その 放射性崩壊の 熱で 光る天体
ResearchResearch themes
相対論と
*Illustrative image中性子星合体からの重力波
中性子星どうしが合体する
*Illustrative imageキロノバ
中性子星の合体で
*Illustrative image合体にともなう電波の残光
合体で
*Illustrative image連星ブラックホールの起源
重力波で
MembersFaculty
- Associate Professor仏坂 健太Publications ↗
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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: “Artist NSIllustration CREDIT NSF LIGO Sonoma State University A. Simonnet” NSF/LIGO/Sonoma State University/A. Simonnet / Public domain (cropped)
- 中性子星合体からの
重力波: “Illustration of Colliding Neutron Stars (2005-grb050709-more-3)” (Illustration: NASA/D.Berry) / Public domain (cropped) - キロノバ: “Illustration of a Kilonova (2022-049)” ARTWORK: NASA, Joseph Olmsted (STScI) / Public domain (cropped)
- 合体に
ともなう 電波の 残光: “VLA Antennas” The Modern Polymath / CC BY-SA 4.0 (cropped) - 連星ブラックホールの
起源: “MergingBinaryBlackHoles” NASA/Ames Research Center/Christopher E. Henze / Public domain (cropped)
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