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Wyświetlanie 1-6 z 6
Tytuł:
Decision theory under general uncertainty
Autorzy:
Cui, Y.
Guo, R.
Dunne, T.
Guo, D.
Tematy:
statistical decision
state space
action space
uncertain measure
loss function
risk
uncertainty decision
Pokaż więcej
Wydawca:
Uniwersytet Morski w Gdyni. Polskie Towarzystwo Bezpieczeństwa i Niezawodności
Powiązania:
https://bibliotekanauki.pl/articles/2069606.pdf  Link otwiera się w nowym oknie
Opis:
The exposure of Toyota management’s cover-up of its faulty car component problems raises a fundamental question: did Toyota management make an appropriate decision taking all uncertainties into account? Statistical decision theory is a framework with a probabilistic foundation, which admits random uncertainty about the real world and human thinking. In general, the uncertainty of the real world is diversified and therefore the effort of trying to deal with different forms of uncertainty with one special form of uncertainty, namely random uncertainty, may be oversimplified. In this paper, we introduce an axiomatic uncertain measure theoretical framework and explore the essential mechanism in formulating a general uncertainty decision theory. We expect that a new understanding of uncertainty and development of a corresponding new uncertainty decision-making approach may assist intelligence communities to survive and deal with the extremely tough and diverse aspects of an uncertain reality.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Random fuzzy continuous-time Markov chains
Autorzy:
Guo, R.
Nyirenda, J.
Dunne, T.
Guo, D.
Tematy:
stochastic semigroup
rate matrix
credibility measure
repairable system
random fuzzy Markov process
Pokaż więcej
Wydawca:
Uniwersytet Morski w Gdyni. Polskie Towarzystwo Bezpieczeństwa i Niezawodności
Powiązania:
https://bibliotekanauki.pl/articles/2069696.pdf  Link otwiera się w nowym oknie
Opis:
Continuous-time Markov chains is an important subclass in stochastic processes, which have facilitated many applications in business decisions, investment risk analysis, insurance policy making and reliability modeling. It should be fully aware that the existing continuous-time Markov chains theory is merely an ideology under which the random uncertainty governs the phenomena. However, the real world phenomena are often revealing the randomness and vagueness co-existence reality and thus the probabilistic continuous-time Markov chains modeling practices may be not adequate. In this paper, we define the random fuzzy continuous-time Markov chains, explore the related average chance distributions, and propose a scheme for the parameter estimation and a simulation scheme as well. It is expecting that a foundational work can be established for reliability modeling and risk analysis, particularly, repairable system modeling.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
The HIBEAM instrument at the European spallation source
Autorzy:
Henriksson, H.
Milstead, D.
Dunne, K.
Pasechnik, R.
Golubev, P.
Putignano, O.
Kozela, A.
Oskarsson, A.
Wolke, M.
Nilsson, T.
Womersley, J.
Kickulies, M.
Holl, M.
Bentley, P.
Santoro, V.
Lee, W. T.
Eriksson, H.
Yiu, S. C.
Heinz, A.
Rogers, J.
Guedes, G. P.
Broussard, L.
Muhrer, G.
Hehl, V.
Burgman, A.
Stadnik, Y. V.
Wagner, R.
Björk, L.
de la Cour, N.
Luzin, G.
Ripa, A.
Amaral, J.
Johansson, H. T.
Nepomuceno, A.
Barrow, J.
Bartis, M.
Ferreira, M. J.
Pałasz, Tadeusz
Åstrand, L.
Snow, W. M.
Jönsson, B.
Marquez Damian, J. I.
Scioscioli, F.
Kamyshkov, Y.
Quirino, T.
Croci, G.
Gorini, G.
Muraro, A.
Rataj, B.
Persson, L. B.
Zanini, L.
Kemp, E.
Kolevatov, R.
Pysz, K.
Brooijmans, G.
Friman-Gayer, U.
Silverstein, S.
Meirose, B.
Lejon, W.
Fierlinger, P.
Di Julio, D. D.
Opis:
The European spallation source (ESS) will be the world's brightest neutron source and will open a new intensity frontier in particle physics. The HIBEAM collaboration aims to exploit the unique potential of the ESS with a dedicated ESS instrument for particle physics which offers world-leading capability in a number of areas. The HIBEAM program includes the first search in thirty years for free neutrons converting to antineutrons and searches for sterile neutrons, ultralight axion dark matter and nonzero neutron electric charge. This paper outlines the capabilities, design, infrastructure, and scientific potential of the HIBEAM program, including its dedicated beamline, neutron optical system, magnetic shielding and control, and detectors for neutrons and antineutrons. Additionally, we discuss the long-term scientific exploitation of HIBEAM, which may include measurements of the neutron electric dipole moment and precision studies of neutron decays.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Autorzy:
Lindroos, M.
Zerzion, D.
Bouquerel, E.
Johansson, H.T.
Wurtz, J.
Markaj, G.
Poussot, P.
Klinkby, E.
Zimmer, O.
Dunne, K.
Saiang, D.
Vankova-Kirilova, G.
Topaksu, A. Kayis
Cupiał, P.
Johansson, R.
Gomez-Cadenas, J.J.
Dracos, M.
Gålnander, B.
Cirigliano, V.
Heil, P.
Kolevatov, R.
Barron-Pálos, L.
Geralis, Th.
Monrabal, F.
Barrow, J.
Johansson, T.
Halić, L.
Brooijmans, G.
Alekou, A.
Danared, H.
Herde, H.
Kliček, B.
Fierlinger, P.
Martins, C.
Rataj, B.
Kildetoft, B.
Krhač, K.
Bodek, Kazimierz
Rozpędzik, Dagmara
Tarkeshian, R.
Larizgoitia, L.
Fynbo, H.O.U.
Konrad, G.
Blanco, C.
Efthymiopoulos, I.
Marrelli, C.
Eklund, L.
Di Julio, D.D.
Algora, A.
Piegsa, F.M.
Wagner, R.
Holl, M.
Kozioł, M.
Snow, W.M.
D’Alessi, L.
Kirch, K.
Oglakci, M.
Frank, A.
Broussard, L.J.
Eshraqi, M.
Milstead, D.
Schober, H.
Nesvizhevsky, V.
Lychagin, E.
Theroine, C.
Bentley, P.
Thorne, J.
Trachanas, E.
Fukuda, T.
Soldner, T.
Degenkolb, S.
Buchan, O.
Yiu, S.C.
Tolba, T.
Fertl, M.
Uggerhøj, U.I.
Carlile, C.J.
Delahaye, J.P.
Märkisch, B.
Bohm, C.
Zanini, L.
Lewis, C.M.
Burgman, A.
Park, J.
Perrey, H.
Takibayev, A.
Abele, H.
Zormpa, O.
Chanel, E.
Petkov, G.
Christiansen, P.
Simón, A.
Milas, N.
Baeßler, S.
Schmidt, U.
Silverstein, S.
Szybiński, B.
Kupść, A.
Lytken, E.
Bijnens, J.
Ekelöf, T.
Kamyshkov, Y.
Olvegård, M.
Mezzetto, M.
Santoro, V.
Cederkall, J.
Collar, J.I.
Łacny, Ł.
Oskarsson, A.
Happe, C.
Schulthess, I.
Morales, E. Cristaldo
Snamina, J.
Muhrer, G.
Ries, D.
Gonzalez, F.
de André, J.P.A.M.
Novella, P.
Fernandez-Martinez, E.
Nepomuceno, A.
Nilsson, T.
Tsenov, R.
Fanourakis, G.
Gazis, N.
Thomas, J.
Friman-Gayer, U.
Zejma, Jacek
Andersen, K.
Patrzalek, D.
Gonzalez-Alonso, M.
Fratangelo, A.
Torres-Sánchez, P.
Tang, Z.
Collins, M.
Baussan, E.
Rizzi, N.
Yoon, S.G.
Wildner, E.
Sosa, A. Garcia
Farricker, A.
Young, A.R.
Damian, J.I. M.
Rosauro-Alcaraz, S.
Stavropoulos, G.
Jericha, E.
Dancila, D.
Berezhiani, Z.
Ota, T.
Marciniewski, P.
Jenke, T.
Ohlsson, T.
Bianchi, A.
Gokbulut, G.
Crawford, C.B.
Bhattacharyya, A.K.
Ferreira, M.J.
Pistillo, C.
Wolke, M.
Zou, Y.
Kraljevic, N. Blaskovic
Ghosh, M.
Vassilopoulos, N.
Sina, H.
Heinz, A.
Wang, X.
Privitera, P.
Folsom, B.
Calén, H.
Esteban, I.
Jenssen, M.
Bolling, B.
Bogomilov, M.
Stipčević, M.
Beßler, Y.
Meirose, B.
Terranova, F.
Persoz, M.
Blennow, M.
Maiano, C.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Supernova model discrimination with Hyper-Kamiokande
Autorzy:
Mineev, O.
Minakata, H.
Nakayoshi, K.
Gialanella, L.
Zaldivar, B.
Kato, A.
Kim, S. Y.
Ashida, Y.
Wilkes, R. J.
Garode, S.
Feng, J.
Vilela, C.
Pac, M. Y.
Karlen, D.
Suganuma, T.
Kajita, T.
Paganini, P.
Lu, X.
Gramegna, F.
Nakadaira, T.
Yano, T.
Ostrowski, Michał
Vivolo, D.
Matusiak, M.
Fiorillo, G.
Mazzucato, E.
Finch, A.
Hiraide, K.
Navarro-Garcia, B.
Mondal, T.
Ikeda, M.
Insler, J.
Kudenko, Y.
Sato, K.
Kumita, T.
Malinský, M.
Lamers James, M.
Nascimento Machado, L.
Wronka, S.
Ohta, K.
Iijima, T.
Gornea, R.
Maret, L.
Jeon, S. H.
Lim, I. T.
Fiorentini, A.
Matsumoto, R.
O'Connor, E.
Coleman, J.
Harada, M.
Kikawa, T.
Danilov, M.
Kearns, E.
Yamaguchi, Y.
Magaletti, L.
Cartwright, S. L.
Nishimura, Y.
Jang, J. S.
Radicioni, E.
Vasseur, G.
Barr, G.
Porwit, K.
Nakagiri, K.
La Commara, M.
Learned, J. G.
Hirota, S.
Marchi, T.
Mollo, C. M.
Di Palma, I.
Sakashita, K.
Izmaylov, A.
El Hedri, S.
Tsukamoto, T.
Ochoa-Ricoux, J. P.
Takemoto, Y.
Medhi, A.
Bonavera, L.
Hartz, M.
Pozimski, J.
Zakrzewski, T.
Chabera, M.
Kinoshita, T.
Stankevich, K. L.
Payne, D.
Renner, J.
Doyle, T. A.
Sashima, I.
Matsuno, S.
Takenaka, A.
Loverre, P.
Wachala, T.
Gumplinger, P.
Booth, N.
Onishchuk, Y.
Ichikawa, A. K.
Ovsiannikova, T.
Suzuki, A. T.
Kameda, J.
Sano, S.
Yoo, J.
Nakai, S.
Hartfiel, B.
Jiang, M.
Moon, C. S.
Pari, M.
Jamieson, B.
Hoshina, K.
Nakajima, Y.
Feusels, T.
Ruggles, C.
Drapier, O.
Prouse, N. W.
Kurjata, R.
Mefodiev, A.
Sekiguchi, T.
Aushev, V.
Labarga, L.
Blanchet, A.
Uchida, Y.
Berardi, V.
Yokoyama, M.
Evangelisti, A.
Kormos, L. L.
Yeum, D. N.
Wendell, R. A.
Iacob, F.
Ogawa, N.
O'Sullivan, E.
Yamamoto, K.
Itow, Y.
Boyd, S. B.
Pasternak, J.
Ruggeri, A. C.
Ozaki, H.
Boiano, A.
Smy, M. B.
Roth, S.
Kim, S. B.
Ferrazzi, B.
Xie, Z.
Xin, T.
Stellacci, S. M.
Fukuda, Y.
Kouzakov, K. A.
Kim, J. H.
Sobczyk, J.
Drakopoulou, E.
Miki, S.
De la Fuente, E.
Munteanu, L.
Yu, M.
Hernando-Morata, J. A.
Longhin, A.
Orozco-Luna, F.
Zarnecki, G.
Korzenev, A.
Spina, R.
Lamoureux, M.
Mongelli, M.
Tzanov, M.
Ioannisian, A.
Cafagna, F. S.
Mermod, P.
González-Nuevo, J.
Carroll, A.
Garde, C.
Grella, G.
Bernardini, E.
Palladino, V.
Kravchuk, L.
Boschi, T.
Playfer, S.
Tanaka, M.
Suvorov, S.
Rountree, S. D.
Aihara, H.
Buchowicz, A.
Ameli, F.
Akutsu, R.
Hassani, S.
Mahn, K.
Fernández-Martinez, E.
Cicerchia, M.
Barker, G. J.
Martin, D.
Idrissi Ibnsalih, W.
Anghel, I.
Fernandez, P.
Jonsson, P.
Cook, L.
Ishida, T.
Wark, D.
Martin, J. F.
Borjabad, S.
Checchia, C.
Seo, J. W.
Lindner, T.
Pavin, M.
Mora, F. J.
Miura, M.
Mellet, L.
Russo, S.
Sobel, H. W.
Taketa, A.
Ziembicki, M.
Khotjantsev, A.
Nakahata, M.
Di Meo, P.
Fujii, Y.
Daz Lopez, G.
Riccio, C.
Wilson, J. R.
Ito, S.
Marinelli, A.
Jang, H. I.
Shimizu, I.
Collazuol, G.
Finley, C.
Niewczas, K.
Gorin, A.
Berns, L.
Antonova, M.
Guigue, M.
Densham, C. J.
Sarmah, P.
Poutissou, J. -M.
Bozza, C.
McGrew, C.
Calabria, N. F.
Ito, H.
Bhadra, S.
Peña-Garay, C.
Shiozawa, M.
Skwarczynski, K.
Mariani, C.
Kakuno, H.
Magar, K.
Konaka, A.
Galinski, G.
Ludovici, L.
Taani, M.
Yen, S.
Friend, M.
Shaykina, A.
Cuen-Rochin, S.
Soler, F. J. P.
Jakkapu, M.
Mezzetto, M.
Murase, K.
Pointon, B. W.
Miller, E. W.
Marti, Ll.
Shin, C. D.
Dumarchez, J.
Kryukov, A. P.
Kasperek, J.
Ishidoshiro, K.
Nakamura, KI.
Pastore, C.
Inomoto, M.
Gomez-Cadenas, J. J.
Suárez Gómez, S. L.
Kisiel, J.
Lee, J.
Popov, A.
Patel, D. A.
Vijayvargi, A.
Ellis, J.
Joo, K. K.
Khabibullin, M.
Suzuki, Y.
Grassi, M.
Minamino, A.
Svoboda, R.
Malek, M.
Walker, J.
Zalipska, J.
Menjo, H.
Rubbia, A.
Fitton, M.
Rajda, P. J.
Shinoki, M.
Valentino, V.
Tada, M.
Santucci, G.
Horiuchi, S.
Giganti, C.
Mehta, P.
Seo, S. H.
Kotsar, Y.
Vyalkov, M. M.
Holin, A.
Choubey, S.
Studenikin, A. I.
Quiroga, A. A.
Esmaili, A.
Ishino, H.
Bronner, C.
Kobayashi, T.
Bravo-Berguño, D.
Okumura, K.
Radics, B.
Koshio, Y.
Cao, S.
Ishitsuka, M.
Long, K. R.
Sgalaberna, D.
Makida, Y.
Vagins, M. R.
Monrabal, F.
Di Lodovico, F.
Bolognesi, S.
Bose, D.
Kazarian, N.
Kalaczynski, P.
Pinzon Guerra, E.
Esteve, R.
Kataoka, Y.
Ogitsu, T.
Takeuchi, Y.
Stopa, K.
Kano, Y.
Parsa, S.
Asaoka, Y.
Deshmukh, N.
Blaszczyk, F. d. M.
Hastings, N. C.
Quilain, B.
Suzuki, S. Y.
Koga, M.
Litchfield, R. P.
Richards, B.
Feely, M.
Laveder, M.
McCarthy, M.
Tortone, G.
Rondio, E.
Migliozzi, P.
Kwak, K.
Inoue, K.
Przewlocki, P.
Abe, K.
Naseby, C. E. R.
Nakaya, T.
Pronost, G.
Takhistov, V.
Metelko, C.
Bellato, M.
Popov, B.
Rychter, A.
de Perio, P.
Sonoda, Y.
Nakamura, H.
Frankiewicz, K.
Bian, J.
Batkiewicz-Kwasniak, M.
Hill, J.
Nicholls, T.
Yershov, N.
Nakayama, S.
Lagoda, J.
Santos, J. D.
Spisso, B.
Pidcott, C.
Roskovec, B.
Bubak, A.
Tomatani-Sánchez, A. K.
Zsoldos, S.
Izumi, N.
Sinnis, G.
Moharana, R.
Sánchez, M. L.
Bravar, A.
Dunne, P.
Ferrario, P.
Scott, M.
Obrebski, W.
Retiere, F.
Kikec, M.
Dergacheva, A.
Alekseev, I.
Gonin, M.
Gao, J.
Bandac, I.
Hadley, D. R.
Samani, S.
Anthony, L. H. V.
Rott, C.
O'Keeffe, H. M.
Noah, E.
Skrobova, N.
Migenda, J.
Hayato, Y.
Araya, A.
Nakamura, K.
Eklund, L.
Suwa, Y.
Tanaka, H. I.
Leitner, R.
Fedotov, S.
Ryu, D.
Garfagnini, A.
Kowalik, K. L.
De Rosa, G.
King, S.
Xia, J.
Blondel, A.
Kutter, T.
Spradlin, P.
Bernard, L.
Chakraborty, S.
Emery, S.
Ospina, N.
Pastuszak, G.
Bergevin, M.
Catanesi, M. G.
Koch, L.
Kolev, N.
Ziętara, Krzysztof
Jo, H. S.
Nagao, Y.
Lawe, M.
Okamoto, K.
Ballester, F.
Maekawa, Y.
Iwamoto, K.
Cebriàn, S.
Ricciardi, G.
Zaremba, K.
Mueller, Th. A.
Rescigno, M.
Moon, D. H.
Matsubara, T.
Dziewiecki, M.
Herrero, V.
Oyama, Y.
Zito, M.
Cowan, G.
Tanaka, H.
Dealtry, T.
Koerich, L.
Stawarz, Łukasz
Yu, I.
Jenkins, S. J.
Yonenaga, M.
Lavitola, L.
Needham, M.
Calvo-Mozota, J. M.
Buizza Avanzini, M.
Ali, A.
Moriyama, S.
Sanchez, M. C.
Adrich, P.
Thiesse, M.
Tsui, K. M.
Vinning, W. G. S.
Yanagisawa, C.
Kuze, M.
Brown, L.
Sánchez, F.
Wilking, M. J.
Klekotko, A.
Gousy-Leblanc, V.
Lezaun, V.
McElwee, J.
Choi, J. H.
O'Sullivan, L.
Mitra, A.
Takeda, A.
Thompson, L. F.
Tanaka, H. A.
Mijakowski, P.
Kim, J. Y.
Paolone, V.
Sekiya, H.
Nova, F.
Seiya, Y.
Mine, S.
Shan, Z.
Nakano, Y.
Katori, T.
Barbi, M.
Marzec, J.
Rose, H. J.
Posiadala-Zezula, M.
McCauley, N.
Wascko, M. O.
Oshlianskyi, A.
Nugent, J. C.
Martens, K.
Nunokawa, H.
Svirida, D.
Hultqvist, K.
Shaikhiev, A.
Devi, M. M.
Vladisavljevic, T.
Tashiro, T.
Toledo, J.
Vogelaar, R. B.
Izumiyama, S.
Valder, S.
Opis:
Core-collapse supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants—neutron stars and black holes—are interesting astrophysical objects in their own right. However, despite millennia of observations and almost a century of astrophysical study, the explosion mechanism of core-collapse supernovae is not yet well understood. Hyper-Kamiokande is a next-generation neutrino detector that will be able to observe the neutrino flux from the next galactic core-collapse supernova in unprecedented detail. We focus on the first 500 ms of the neutrino burst, corresponding to the accretion phase, and use a newly-developed, high-precision supernova event generator to simulate Hyper-Kamiokande's response to five different supernova models. We show that Hyper-Kamiokande will be able to distinguish between these models with high accuracy for a supernova at a distance of up to 100 kpc. Once the next galactic supernova happens, this ability will be a powerful tool for guiding simulations toward a precise reproduction of the explosion mechanism observed in nature.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
    Wyświetlanie 1-6 z 6

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