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吉田 至順 研究室
Showing the original Japanese · View translation
磁場を持つ中性子星の平衡形状と性質を理論で解き明かす研究室。
AboutAbout the lab
磁場を持つ中性子星を、理論で描き出す。
吉田 至順 研究室は、
中性子星は、
一般相対論の
Key terms
- 中性子星
- 高エネルギー天体現象の
中心天体と 考えられている 天体の 一つ。 内部の 構造、 特に 磁場の 理解は まだ 十分でない - 磁気中性子星
- 磁場を
伴った 中性子星。 この 研究室では、 その 平衡形状を 一般相対論の 理論で 調べている - 平衡解
- 星が
形を 保って 釣り合っている 状態を 表す、 方程式の 解。 安定性を 調べる 出発点に なる
ResearchResearch themes
中性子星の
MembersFaculty
- Assistant Professor吉田 至順
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: “The Star with a Secret Identity” X-ray: NASA/CXC/Huntingdon Inst. for X-ray Astronomy/G.Garmire, Optical: ESO/VLT / Public domain (cropped)
- 一般相対論的な
磁気中性子星の 平衡形状: “Artist’s impression of the magnetar in the star cluster Westerlund 1” ESO/L. Calçada / CC BY 4.0 (cropped) - Related lab (當真 賢二 研究室): “Artist’s illustration of galaxy with jets from a supermassive black hole” ESA/Hubble, L. Calçada (ESO) / CC BY 4.0 (cropped)
- Related lab (藤林 翔 研究室): “Vela Supernova Remnant - Noirlab2406a” CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab) / CC BY 4.0 (cropped)
- Related lab (野田 博文 研究室): “Chandra X-Ray Observatory (noirlab2427c)” NASA/CXC & J.Vaughan / CC BY 4.0 (cropped)
- Related lab (木村 成生 研究室): “Anatomy of an Active Galactic Nucleus (SVS14922 - Jet illustrated Loop v01 00001 print)” NASA's Scientific Visualization Studio - NASA’s Goddard Space Flight Center’s Conceptual Image Lab / Public domain (cropped)
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