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Institution

Fukuoka Institute of Technology

EducationFukuoka, Japan
About: Fukuoka Institute of Technology is a education organization based out in Fukuoka, Japan. It is known for research contribution in the topics: Node (networking) & Wireless mesh network. The organization has 1276 authors who have published 3729 publications receiving 33299 citations. The organization is also known as: Fukuoka kōgyō daigaku.


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Book ChapterDOI
01 Jan 2014
TL;DR: In this paper, the authors describe the story of the recent developments and the future perspectives in physics of liquid crystals, especially focusing on the contributions by Japanese research groups for the last decade, and present new subjects unmentioned in the book.
Abstract: Over the 100 years since its discovery, liquid crystals have been the intriguing subject for both academia and industries. The textbook of de Gennes The Physics of Liquid Crystals published in 1974 is still the bible for many LC researchers, but new subjects unmentioned in the book have also risen for these years. This chapter describes the story of the recent developments and the future perspectives in physics of liquid crystals, especially focusing on the contributions by Japanese research groups for the last decade.

2,005 citations

Journal ArticleDOI
K. Abe1, Y. Hayato1, T. Iida1, M. Ikeda1, M. Ikeda2, C. Ishihara1, K. Iyogi1, J. Kameda1, Ken-ichiro Kobayashi1, Yusuke Koshio1, Y. Kozuma1, M. Miura1, S. Moriyama1, Masayuki Nakahata1, S. Nakayama1, Y. Obayashi1, H. Ogawa1, Hiroyuki Sekiya1, Masato Shiozawa1, Yasunari Suzuki1, Atsushi Takeda1, Y. Takenaga1, Koh Ueno1, K. Ueshima, Hiroshi Watanabe, S. Yamada1, T. Yokozawa1, S. Hazama1, H. Kaji1, Takaaki Kajita1, K. Kaneyuki1, T. McLachlan1, Ko Okumura1, Y. Shimizu1, N. Tanimoto1, M. R. Vagins3, M. R. Vagins1, L. Labarga4, L. M. Magro4, Frédéric Dufour5, E. Kearns5, E. Kearns1, Michael Litos5, J. L. Raaf5, J. L. Stone5, J. L. Stone1, L. R. Sulak5, W. Wang6, W. Wang5, M. Goldhaber7, K. Bays3, David William Casper3, J. P. Cravens3, W. R. Kropp3, S. Mine3, C. Regis3, A. L. Renshaw3, M. B. Smy1, M. B. Smy3, H. W. Sobel3, H. W. Sobel1, K. S. Ganezer8, John Hill8, W. E. Keig8, J. S. Jang9, J. Y. Kim9, I. T. Lim9, Justin Albert10, R. A. Wendell10, T. Wongjirad10, Kate Scholberg10, Kate Scholberg1, C. W. Walter1, C. W. Walter10, T. Ishizuka11, S. Tasaka12, John G. Learned, S. Matsuno, Y. Watanabe13, Takehisa Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, Koji Nakamura1, K. Nishikawa, H. Nishino, Yuichi Oyama, Ken Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki14, Y. Takeuchi14, Y. Takeuchi1, A. Minamino2, Tsuyoshi Nakaya1, Tsuyoshi Nakaya2, Y. Fukuda15, Yoshitaka Itow16, G. Mitsuka16, T. Tanaka16, C. K. Jung17, G. D. Lopez17, C. McGrew17, R. Terri17, C. Yanagisawa17, N. Tamura18, Hirokazu Ishino19, A. Kibayashi19, S. Mino19, Takaaki Mori19, Makoto Sakuda19, H. Toyota19, Y. Kuno20, Minoru Yoshida20, S. B. Kim21, B. S. Yang21, H. Okazawa22, Y. Choi23, K. Nishijima24, Y. Yokosawa24, M. Koshiba1, Y. Totsuka1, Masashi Yokoyama1, Song Chen25, Y. Heng25, Zishuo Yang25, Haoxiong Zhang25, D. Kielczewska26, P. Mijakowski26, K. Connolly27, M. Dziomba27, E. Thrane27, E. Thrane28, R. J. Wilkes27 
TL;DR: The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results in this article, where improved detector calibrations, a full detector simulation, and improved analysis methods are estimated to be approximately 2.1%, which is about two thirds of the systematic uncertainty for the first phase.
Abstract: The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results. With improved detector calibrations, a full detector simulation, and improved analysis methods, the systematic uncertainty on the total neutrino flux is estimated to be $\ifmmode\pm\else\textpm\fi{}2.1%$, which is about two thirds of the systematic uncertainty for the first phase of Super-Kamiokande. The observed $^{8}\mathrm{B}$ solar flux in the 5.0 to 20 MeV total electron energy region is $2.32\ifmmode\pm\else\textpm\fi{}0.04(\mathrm{stat})\ifmmode\pm\else\textpm\fi{}0.05(\mathrm{sys})\ifmmode\times\else\texttimes\fi{}{10}^{6}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{sec}}^{\ensuremath{-}1}$ under the assumption of pure electron-flavor content, in agreement with previous measurements. A combined oscillation analysis is carried out using SK-I, II, and III data, and the results are also combined with the results of other solar neutrino experiments. The best-fit oscillation parameters are obtained to be ${sin }^{2}{\ensuremath{\theta}}_{12}={0.30}_{\ensuremath{-}0.01}^{+0.02}({tan }^{2}{\ensuremath{\theta}}_{12}={0.42}_{\ensuremath{-}0.02}^{+0.04})$ and $\ensuremath{\Delta}{m}_{21}^{2}={6.2}_{\ensuremath{-}1.9}^{+1.1}\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}\text{ }\text{ }{\mathrm{eV}}^{2}$. Combined with KamLAND results, the best-fit oscillation parameters are found to be ${sin }^{2}{\ensuremath{\theta}}_{12}=0.31\ifmmode\pm\else\textpm\fi{}0.01({tan }^{2}{\ensuremath{\theta}}_{12}=0.44\ifmmode\pm\else\textpm\fi{}0.03)$ and $\ensuremath{\Delta}{m}_{21}^{2}=7.6\ifmmode\pm\else\textpm\fi{}0.2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}\text{ }\text{ }{\mathrm{eV}}^{2}$. The $^{8}\mathrm{B}$ neutrino flux obtained from global solar neutrino experiments is $5.3\ifmmode\pm\else\textpm\fi{}0.2(\mathrm{stat}+\mathrm{sys})\ifmmode\times\else\texttimes\fi{}{10}^{6}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}$, while the $^{8}\mathrm{B}$ flux becomes $5.1\ifmmode\pm\else\textpm\fi{}0.1(\mathrm{stat}+\mathrm{sys})\ifmmode\times\else\texttimes\fi{}{10}^{6}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}$ by adding KamLAND results. In a three-flavor analysis combining all solar neutrino experiments, the upper limit of ${sin }^{2}{\ensuremath{\theta}}_{13}$ is 0.060 at 95% C.L.. After combination with KamLAND results, the upper limit of ${sin }^{2}{\ensuremath{\theta}}_{13}$ is found to be 0.059 at 95% C.L.

404 citations

Journal ArticleDOI
K. Choi1, K. Abe2, K. Abe3, Yoshinori Haga3, Y. Hayato3, Y. Hayato2, K. Iyogi3, J. Kameda2, J. Kameda3, Yasuhiro Kishimoto3, Yasuhiro Kishimoto2, M. Miura3, M. Miura2, S. Moriyama2, S. Moriyama3, Masayuki Nakahata2, Masayuki Nakahata3, Yuuki Nakano3, S. Nakayama3, S. Nakayama2, Hiroyuki Sekiya2, Hiroyuki Sekiya3, Masato Shiozawa3, Masato Shiozawa2, Yasunari Suzuki2, Yasunari Suzuki3, Atsushi Takeda2, Atsushi Takeda3, T. Tomura2, T. Tomura3, R. A. Wendell3, R. A. Wendell2, T. J. Irvine3, Takaaki Kajita3, Takaaki Kajita2, I. Kametani3, K. Kaneyuki2, K. Kaneyuki3, K. P. Lee3, Y. Nishimura3, Kimihiro Okumura2, Kimihiro Okumura3, T. McLachlan3, L. Labarga, E. Kearns2, E. Kearns4, J. L. Raaf4, J. L. Stone2, J. L. Stone4, L. R. Sulak4, S. Berkman5, H.A. Tanaka5, S. Tobayama5, M. Goldhaber6, G. Carminati7, W. R. Kropp7, S. Mine7, A. L. Renshaw7, M. B. Smy7, M. B. Smy2, H. W. Sobel2, H. W. Sobel7, K. S. Ganezer8, John Hill8, N. Hong9, J. Y. Kim9, I. T. Lim9, T. Akiri10, A. Himmel10, Kate Scholberg2, Kate Scholberg10, C. W. Walter10, C. W. Walter2, T. Wongjirad10, T. Ishizuka11, Shigeki Tasaka12, J. S. Jang13, J. G. Learned14, S. Matsuno14, S. N. Smith14, T. Hasegawa15, T. Ishida15, T. Ishii15, T. Kobayashi15, T. Nakadaira15, K. Nakamura2, K. Nakamura15, Yuichi Oyama15, K. Sakashita15, T. Sekiguchi15, T. Tsukamoto15, A. T. Suzuki16, Y. Takeuchi16, C. Bronner17, Seiko Hirota17, K. Huang17, K. Ieki17, M. Ikeda17, T. Kikawa17, A. Minamino17, Tsuyoshi Nakaya2, Tsuyoshi Nakaya17, Kazuhiro Suzuki17, Susumu Takahashi17, Y. Fukuda18, Yoshitaka Itow1, G. Mitsuka1, P. Mijakowski, Joshua Hignight19, J. Imber19, C. K. Jung19, C. Yanagisawa19, Hirokazu Ishino20, A. Kibayashi20, Yusuke Koshio20, Takaaki Mori20, Makoto Sakuda20, T. Yano20, Y. Kuno21, R. Tacik22, R. Tacik23, S. B. Kim24, H. Okazawa25, Y. Choi26, K. Nishijima27, M. Koshiba3, Y. Totsuka3, Masashi Yokoyama3, Masashi Yokoyama2, K. Martens2, Ll. Marti2, M. R. Vagins7, M. R. Vagins2, J. F. Martin28, P. de Perio28, A. Konaka22, M. J. Wilking22, Song Chen29, Yejin Zhang29, R. J. Wilkes30 
TL;DR: In this article, the authors considered neutrino events with interaction vertices in the SK detector in addition to upward-going muons produced in the surrounding rock and found no significant excess over expected atmospheric-neutrino background and interpreted the result in terms of upper limits on WIMP-nucleon elastic scattering cross sections under different assumptions about the annihilation channel.
Abstract: Super-Kamiokande (SK) can search for weakly interacting massive particles (WIMPs) by detecting neutrinos produced from WIMP annihilations occurring inside the Sun. In this analysis, we include neutrino events with interaction vertices in the detector in addition to upward-going muons produced in the surrounding rock. Compared to the previous result, which used the upward-going muons only, the signal acceptances for light (few-GeV/c^{2}-200-GeV/c^{2}) WIMPs are significantly increased. We fit 3903 days of SK data to search for the contribution of neutrinos from WIMP annihilation in the Sun. We found no significant excess over expected atmospheric-neutrino background and the result is interpreted in terms of upper limits on WIMP-nucleon elastic scattering cross sections under different assumptions about the annihilation channel. We set the current best limits on the spin-dependent WIMP-proton cross section for WIMP masses below 200 GeV/c^{2} (at 10 GeV/c^{2}, 1.49×10^{-39} cm^{2} for χχ→bb[over ¯] and 1.31×10^{-40} cm^{2} for χχ→τ^{+}τ^{-} annihilation channels), also ruling out some fraction of WIMP candidates with spin-independent coupling in the few-GeV/c^{2} mass range.

297 citations

Journal ArticleDOI
TL;DR: The discovery and development of catalysts and catalytic processes are essential components to maintaining an ecological balance in the future as mentioned in this paper, and recent revolutions made in data science could have a...
Abstract: The discovery and development of catalysts and catalytic processes are essential components to maintaining an ecological balance in the future. Recent revolutions made in data science could have a ...

272 citations

Journal ArticleDOI
TL;DR: The antioxidant properties of brown algal phlorotannins were evaluated using the inhibition of phospholipid peroxidation in the liposome system, and by determining radical scavenging activities against the superoxide anion and 1,1-diphenyl-2-picrylhydrazyl (DPPH) as discussed by the authors.
Abstract: The antioxidant activities of brown algal phlorotannins were evaluated using the inhibition of phospholipid peroxidation in the liposome system, and by determining radical scavenging activities against the superoxide anion and 1,1-diphenyl-2-picrylhydrazyl (DPPH). Oligomers of phloroglucinol (1,3,5-trihydroxybenzene), eckol (a trimer), phlorofucofuroeckol A (a pentamer), dieckol and 8,8′-bieckol (hexamers), isolated from the Laminarian brown algae Eisenia bicyclis, Ecklonia cava and Ecklonia kurome, showed potent inhibition of phospholipid peroxidation at 1 μM in the liposome system. The phlorotannins had significant radical scavenging activities against the superoxide anion (50% effective concentration values: 6.5–8.4 μM) and DPPH (50% effective concentration values: 12–26 μM), and were more effective compared to ascorbic acid and α-tocopherol. For the purpose of using phlorotannins as functional food ingredients, the antioxidant activity of a complex of crude phlorotannins and soybean protein was examined. The complex had a pronounced DPPH-radical scavenging activity. These results suggest that phlorotannins are potent anti-inflammatory substances, and that the Laminariaceous brown algae, which are abundant in phlorotannins, may be useful as a new functional foodstuff or supplement with anti-inflammatory activity.

265 citations


Authors

Showing all 1279 results

NameH-indexPapersCitations
Hiroshi Nishihara6261614683
Fatos Xhafa5269210379
Leonard Barolli4711459969
Makoto Takizawa379398518
Jianjun Zhao362084556
Hiroshi Yasuoka362654511
Nobuyoshi Miyamoto31912602
Makoto Ikeda303853225
Shinji Sakamoto301152108
T. Ishizuka29583224
Kazunori Yoshiura291462092
Hiroshi Nakashima282443576
Rajesh Madhu28472026
Takashi Kamachi28812293
Régis Guégan26851906
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20235
202210
2021155
2020223
2019230
2018229