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Institution

University of Warsaw

EducationWarsaw, Poland
About: University of Warsaw is a education organization based out in Warsaw, Poland. It is known for research contribution in the topics: Population & Large Hadron Collider. The organization has 20832 authors who have published 56617 publications receiving 1185084 citations. The organization is also known as: Uniwersytet Warszawski & Warsaw University.


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Journal ArticleDOI
TL;DR: In this article, a new inequality bounding slopes of the restriction of a sheaf to a hypersurface in terms of its slope and the discriminant was proposed, which implies that the moduli spaces of Gieseker semistable sheaves are projective schemes of finite type.
Abstract: We prove Maruyama’s conjecture on the boundedness of slope semistable sheaves on a projective variety defined over a noetherian ring. Our approach also gives a new proof of the boundedness for varieties defined over a characteristic zero field. This result implies that in mixed characteristic the moduli spaces of Gieseker semistable sheaves are projective schemes of finite type. The proof uses a new inequality bounding slopes of the restriction of a sheaf to a hypersurface in terms of its slope and the discriminant. This inequality also leads to effective restriction theorems in all characteristics, improving earlier results in characteristic zero.

404 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. Smy3, M. B. Smy1, H. W. Sobel1, H. W. Sobel3, 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. Takeuchi1, Y. Takeuchi14, 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. Thrane28, E. Thrane27, 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
TL;DR: Bringing together the combination of modern computational power and algorithms from graph/network theory, chemical rules, and the elements of quantum mechanics, the machine can finally be "taught" how to plan syntheses of non-trivial organic molecules in a matter of seconds to minutes.
Abstract: Exactly half a century has passed since the launch of the first documented research project (1965 Dendral) on computer-assisted organic synthesis. Many more programs were created in the 1970s and 1980s but the enthusiasm of these pioneering days had largely dissipated by the 2000s, and the challenge of teaching the computer how to plan organic syntheses earned itself the reputation of a "mission impossible". This is quite curious given that, in the meantime, computers have "learned" many other skills that had been considered exclusive domains of human intellect and creativity-for example, machines can nowadays play chess better than human world champions and they can compose classical music pleasant to the human ear. Although there have been no similar feats in organic synthesis, this Review argues that to concede defeat would be premature. Indeed, bringing together the combination of modern computational power and algorithms from graph/network theory, chemical rules (with full stereo- and regiochemistry) coded in appropriate formats, and the elements of quantum mechanics, the machine can finally be "taught" how to plan syntheses of non-trivial organic molecules in a matter of seconds to minutes. The Review begins with an overview of some basic theoretical concepts essential for the big-data analysis of chemical syntheses. It progresses to the problem of optimizing pathways involving known reactions. It culminates with discussion of algorithms that allow for a completely de novo and fully automated design of syntheses leading to relatively complex targets, including those that have not been made before. Of course, there are still things to be improved, but computers are finally becoming relevant and helpful to the practice of organic-synthetic planning. Paraphrasing Churchill's famous words after the Allies' first major victory over the Axis forces in Africa, it is not the end, it is not even the beginning of the end, but it is the end of the beginning for the computer-assisted synthesis planning. The machine is here to stay.

403 citations

Journal ArticleDOI
01 Feb 1990-Nature
TL;DR: Experimental data from eight filter-feeding species are presented that strongly support the cornerstone assumption of the competitive aspect of the size-efficiency hypothesis, showing that the threshold food concentration necessary to assure that assimilation equals respiration, is lower for the large-bodied species than it is for the small-bodiedspecies under steady-state and low-mortality conditions.
Abstract: ACCORDING to the size–efficiency hypothesis1, body size is one of the most important determinants of the relative abundance of planktonic animals in nature. First, large-bodied species are more vulnerable to predation by visually feeding planktivorous fishes. Second, they are superior competitors for resources, being able to grow and reproduce at lower food concentrations. But whereas the first assumption has been confirmed by many field and experimental data (for review see refs 2–4), the second suggestion lacks experimental evidence and has been frequently questioned5-12. I now present experimental data from eight filter-feeding species (family Daphnidae) that strongly support the cornerstone assumption of the competitive aspect of the size-efficiency hypothesis. These data show that the threshold food concentration necessary to assure that assimilation equals respiration13, is lower for the large-bodied species than it is for the small-bodied species under steady-state and low-mortality conditions.

402 citations

Journal ArticleDOI
TL;DR: This work carries out state-of-the-art optimization of a nuclear energy density of Skyrme type in the framework of the Hartree-Fock-Bogoliubov (HFB) theory, with new model-based, derivative-free optimization algorithm.
Abstract: We carry out state-of-the-art optimization of a nuclear energy density of Skyrme type in the framework of the Hartree-Fock-Bogoliubov theory. The particle-hole and particle-particle channels are optimized simultaneously, and the experimental data set includes both spherical and deformed nuclei. The new model-based, derivative-free optimization algorithm used in this work has been found to be significantly better than standard optimization methods in terms of reliability, speed, accuracy, and precision. The resulting parameter set unedf0 results in good agreement with experimental masses, radii, and deformations and seems to be free of finite-size instabilities. An estimate of the reliability of the obtained parameterization is given, based on standard statistical methods. We discuss new physics insights offered by the advanced covariance analysis.

402 citations


Authors

Showing all 21191 results

NameH-indexPapersCitations
Alexander Malakhov139148699556
Emmanuelle Perez138155099016
Piotr Zalewski135138889976
Krzysztof Doroba133144089029
Hector F. DeLuca133130369395
Krzysztof M. Gorski132380105912
Igor Golutvin131128288559
Jan Krolikowski131128983994
Michal Szleper130123882036
Anatoli Zarubin129120486435
Malgorzata Kazana129117581106
Artur Kalinowski129116281906
Predrag Milenovic129118581144
Marcin Konecki128117879392
Karol Bunkowski128119279455
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
2023176
2022619
20212,882
20203,208
20193,130
20183,164