Institution
Tokyo Institute of Technology
Education•Tokyo, Tôkyô, Japan•
About: Tokyo Institute of Technology is a education organization based out in Tokyo, Tôkyô, Japan. It is known for research contribution in the topics: Catalysis & Thin film. The organization has 46775 authors who have published 101656 publications receiving 2357893 citations. The organization is also known as: Tokyo Tech & Tokodai.
Topics: Catalysis, Thin film, Laser, Phase (matter), Polymerization
Papers published on a yearly basis
Papers
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TL;DR: The structure of NiO-SrTiO/sub 3/ powder has been studied by spectroscopic methods such as SEM, TEM, EXAFS, XANES, and XPS as mentioned in this paper.
Abstract: The structure of NiO-SrTiO/sub 3/ powder, which is a photocatalyst for the decomposition of water into H/sub 2/ and O/sub 2/, has been studied by spectroscopic methods such as SEM, TEM, EXAFS, XANES, and XPS. It has been clearly shown that the active catalyst has a peculiar structure; that is, nickel metal exists at the interface of NiO and SrTiO/sub 3/. The surface of NiO changes further into Ni(OH)/sub 2/ during the photocatalytic reaction in water. 31 references, 7 figures, 2 tables.
343 citations
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University of Tokyo1, Boston University2, Seoul National University3, KEK4, Brookhaven National Laboratory5, University of California, Irvine6, California State University, Dominguez Hills7, George Mason University8, Gifu University9, Kobe University10, Los Alamos National Laboratory11, Louisiana State University12, University of Maryland, College Park13, University of Chicago14, Miyagi University of Education15, Stony Brook University16, Niigata University17, Shizuoka University18, Osaka University19, Tohoku University20, Tokai University21, Tokyo Institute of Technology22, University of Warsaw23, University of Washington24
TL;DR: In this article, the super-Kamiokande detector was used to detect atmospheric neutrino interactions with momentum p e > 100 MeV/c, p μ > 200 MeV /c, and with visible energy less than 1.33 GeV.
342 citations
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TL;DR: In this article, local structures in ceria-based materials were investigated by UV resonance Raman spectroscopy using a 3638 nm laser line for the first time in the spectra of a highly crystalline and undoped ceria.
Abstract: Local structures in ceria-based materials were investigated by UV resonance Raman spectroscopy using a 3638 nm laser line for the first time In the spectra of a highly crystalline and undoped ceria, overtone LO series are clearly detected due to the multiphonon relaxation by the UV resonance Raman effect Gd3+ doping in ceria additionally activates the disorder bands that are attributable to lattice spaces with or without an oxygen vacancy The crystal size dependency of the UV Raman spectra suggests that Ce3+ ions preferably form the MO8-type (M = Ce3+) complex in the undoped ceria nanoparticles and are eliminated by oxidation while heating in air Gd3+ ions also tend to form a MO8-type complex in the nanocrystalline ceria matrix However, they diffuse to form the more thermodynamically stable defect clusters that accompany the grain growth upon heating
342 citations
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National Institutes of Natural Sciences, Japan1, University of Tokyo2, Kyoto University3, Goddard Space Flight Center4, Osaka City University5, Waseda University6, Hirosaki University7, Columbia University8, Nihon University9, Tokyo Keizai University10, Osaka University11, Tohoku University12, Rikkyo University13, University of Texas at Brownsville14, Shibaura Institute of Technology15, Japan Aerospace Exploration Agency16, National Institute of Advanced Industrial Science and Technology17, Tokai University18, National Institute of Information and Communications Technology19, Kindai University20, University of Wisconsin–Milwaukee21, Ochanomizu University22, Liverpool John Moores University23, Lancaster University24, Hiroshima University25, California Institute of Technology26, University of Electro-Communications27, Rochester Institute of Technology28, National Defense Academy of Japan29, Niigata University30, University of Southampton31, Osaka Institute of Technology32, Albert Einstein Institution33, Aristotle University of Thessaloniki34, Nagoya University35, Nagaoka University of Technology36, University of Illinois at Urbana–Champaign37, Tokyo Institute of Technology38
TL;DR: DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) as discussed by the authors is the future Japanese space gravitational wave antenna, which aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy.
Abstract: DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy. The pre-conceptual design of DECIGO consists of three drag-free satellites, 1000 km apart from each other, whose relative displacements are measured by a Fabry–Perot Michelson interferometer. We plan to launch DECIGO in 2024 after a long and intense development phase, including two pathfinder missions for verification of required technologies.
342 citations
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TL;DR: In this paper, a photocatalytic decomposition of H2O to form H2 and O2 over NiOK4Nb6O17 powder (1-10 μm, band gap = 3.3 eV), which is an ion-exchangeable layered compound, proceeds steadily more than 50 h under the bandgap irradiation.
341 citations
Authors
Showing all 46967 results
Name | H-index | Papers | Citations |
---|---|---|---|
Matthew Meyerson | 194 | 553 | 243726 |
Yury Gogotsi | 171 | 956 | 144520 |
Masayuki Yamamoto | 171 | 1576 | 123028 |
H. Eugene Stanley | 154 | 1190 | 122321 |
Takashi Taniguchi | 152 | 2141 | 110658 |
Shu-Hong Yu | 144 | 799 | 70853 |
Kazunori Kataoka | 138 | 908 | 70412 |
Osamu Jinnouchi | 135 | 885 | 86104 |
Hector F. DeLuca | 133 | 1303 | 69395 |
Shlomo Havlin | 131 | 1013 | 83347 |
Hiroyuki Iwasaki | 131 | 1009 | 82739 |
Kazunari Domen | 130 | 908 | 77964 |
Hideo Hosono | 128 | 1549 | 100279 |
Hideyuki Okano | 128 | 1169 | 67148 |
Andreas Strasser | 128 | 509 | 66903 |