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応答物性 (Y)
Showing the original Japanese · View translation
電場や光を加えたときの物質の「応答」から、新しい物質を生み出す研究室。
AboutAbout the lab
多様な構造に潜む新奇な応答物性を追求する。
応答物性研究室
分極や
結晶・準結晶・
物性物理学の
Key terms
- 分極
- 物質の
中で プラスと マイナスの 電気の 位置が ずれ、 電気的な 偏りが 生じる こと - 誘電率
- 物質に
電場を かけた ときの、 分極の 起こりやすさを 表す量。 コンデンサの 性能に 関わる - 準結晶
- 原子が
規則正しく 並んでいるのに、 結晶の ような 周期的なくり返しを もたない 物質
NewsLab news
修士課程の
学生が、 日本物理学会 学生優秀発表賞を 受賞 博士課程の
学生が、 セラミックス協会関東支部大会で 特別賞を 受賞 新しい
反強誘電体を 発見 （プレスリリース） 修士課程の
学生が、 「超秩序構造科学」 若手の 学校で フォレスト賞を 受賞
ResearchResearch themes
結晶・準結晶・
MembersFaculty
応答物性研究室の
- Professor谷口 博基
- Lecturer出口 和彦
VoicesStudent voices
Compiled from answers by students who were in the lab. Ratings and reviews reflect individual students' experiences, not the lab's official views.
Students who take part in an interview may receive a thank-you gift worth ¥1,000, regardless of what they say.
On a 4-point scale, ● marks where students' answers fall
Who is this lab for?
What's great about this lab?
What did you learn after joining?
What's the vibe, and what is the professor like?
Where do graduates go?
RelatedLabs similar to 応答物性 (Y)
プラズマ理論 (P)理学部 物理学科電磁場と
複雑性科学実験 (ΣE)理学部 物理学科恒星、
銀河進化学 (Ω)理学部 物理学科銀河はThe information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
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: “Dense pellet forming9” Dominik Bejma, Marta Kowalkińska / CC BY-SA 4.0 (cropped)
- 新しい
応答を 示す物質の 設計と 創出: “Perovskite” Cadmium at English Wikipedia / Public domain (cropped) - Related lab (プラズマ理論 (P)): “Cross-section of the Wendelstein 7-X plasma vessel” Siarhei Besarab / CC BY-SA 4.0 (cropped)
- Related lab (複雑性科学実験 (ΣE)): “Experimental hall of the Wendelstein 7-X stellarator at IPP Greifswald 04” Siarhei Besarab / CC BY-SA 4.0 (cropped)
- Related lab (銀河進化学 (Ω)): “UGC 1810 and UGC 1813 in Arp 273 (captured by the Hubble Space Telescope)” NASA, ESA, and the Hubble Heritage Team (STScI/AURA) / Public domain (cropped)
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