Informacja

Drogi użytkowniku, aplikacja do prawidłowego działania wymaga obsługi JavaScript. Proszę włącz obsługę JavaScript w Twojej przeglądarce.

Wyszukujesz frazę "Shin, C. D." wg kryterium: Autor


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
Tytuł:
Ergonomic Hand Tool and Desk and Chair Development Process
Autorzy:
Shin, D.
Kim, J. Y.
Hallbeck, M. S.
Haight, J. M.
Jung, M. C.
Tematy:
ergonomics process
hand tool
desk and chair
Pokaż więcej
Wydawca:
Centralny Instytut Ochrony Pracy
Powiązania:
https://bibliotekanauki.pl/articles/89795.pdf  Link otwiera się w nowym oknie
Opis:
This paper suggests a practical and simple process consisting of 8 stages: needs assessment, ergonomics guidelines, anthropometry, brainstorming and idea sketch, preliminary model, drafting and rendering, working prototype, and user trials. The feasibility of this process was verified with the development of a modified clamping hand tool and a new student desk and chair. The case studies showed how design difficulties were overcome by integrating ergonomics guidelines in the process.
Dostawca treści:
Biblioteka Nauki
Artykuł
Tytuł:
Multimessenger search for exotic field emission with a global magnetometer network
Autorzy:
Shin, Y. C.
Kim, D.
Semertzidis, Y. K.
Peng, X.
Ruimi, O. M.
Park, S. Y.
Klinger, E.
Pustelny, Szymon
Givon, M.
Segura, P. C.
Kimball, D. F. Jackson
Figueroa, N. L.
Buchler, B. C.
Gavilán-Martín, D.
Wickenbrock, A.
Zhang, J.
Hedges, M. P.
Łukasiewicz, Grzegorz
Budker, D.
Stalnaker, J. E.
Kryemadhi, A.
Kornack, T.
Padniuk, Mikhail
Khamis, Sami S.
Wu, T.
Masia-Roig, H.
Guo, H.
Zhao, Y.
Kukowski, N.
Palm, C. A.
Scholtes, T.
Tandon, D.
Wilson, T. Z.
Hamilton, Paul
Afach, S.
Folman, R.
Pospelov, M.
Rosenzweig, Y.
Grujić, Z. D.
Sulai, Ibrahim A.
Weis, A.
Opis:
The history of astronomy has shown that advances in sensing methods open up new windows to the Universe and often lead to unexpected discoveries. Quantum sensor networks in combination with traditional astronomical observations are emerging as a novel modality for multimessenger astronomy. Here we develop a generic analysis framework that uses a data-driven approach to model the sensitivity of a quantum sensor network to astrophysical signals as a consequence of beyond-the-standard model (BSM) physics. The analysis method evaluates correlations between sensors to search for BSM signals coincident with astrophysical triggers, such as black hole mergers, supernovae, or fast radio bursts. Complementary to astroparticle approaches that search for particlelike signals (e.g., weakly interacting massive particles), quantum sensors are sensitive to wavelike signals from exotic quantum fields. This analysis method can be applied to networks of different types of quantum sensors, such as atomic clocks, matter-wave interferometers, and nuclear clocks, which can probe many types of interactions between BSM fields and standard model particles. We use this analysis method to carry out the first direct search utilizing a terrestrial network of precision quantum sensors for BSM fields emitted during a black hole merger. Specifically, we use the global network of optical magnetometers for exotic physics (GNOME) to perform a search for exotic low-mass field (ELF) bursts generated in coincidence with a gravitational-wave signal from a binary black hole merger (GW200311_115853) detected by LIGO/Virgo on the March 11, 2020. The associated gravitational wave heralds the arrival of the ELF burst that interacts with the spins of fermions in the magnetometers. This enables GNOME to serve as a tool for multimessenger astronomy. Our search found no significant events and, consequently, we place the first lab-based limits on combinations of ELF production and coupling parameters.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Search for topological defect dark matter with a global network of optical magnetometers
Autorzy:
Dailey, Conner
Kornack, Thomas
Wang, Tao
Masia-Roig, Hector
Hamilton, Paul S.
Sheng, Dong
Smiga, Joseph A.
Weis, Antoine
Buchler, Ben C.
Jackson Kimball, Derek F.
Grujić, Zoran D.
Stalnaker, Jason E.
Monroy, Madeline
Sulai, Ibrahim
Pustelny, Szymon
Peng, Xiang
Khamis, Sami
Kim, Dongok
Wilson, Tatum
Lebedev, Victor
Wickenbrock, Arne
Hedges, Morgan
Paul, Karun V.
Zhang, Jianwei
Pospelov, Maxim
Padniuk, Mikhail
Budker, Dmitry
Palm, Christopher A.
Derevianko, Andrei
Tandon, Dhruv
Figueroa, Nataniel L.
Gerhardt, Ilja
Segura, Perrin C.
Lu, Zheng-Tian
Afach, Samer
Semertzidis, Yannis K.
Penaflor, Alexander
Wu, Teng
Wurm, David
Yu, Dongrui
Yang, Yucheng
Scholtes, Theo
Dumont, Vincent
Shin, Yun Chang
Park, Sun Yool
Hao, Chuanpeng
Guo, Hong
Preston, Rayshaun
Xiao, Wei
Opis:
Ultralight bosons such as axion-like particles are viable candidates for dark matter. They can form stable, macroscopic field configurations in the form of topological defects that could concentrate the dark matter density into many distinct, compact spatial regions that are small compared with the Galaxy but much larger than the Earth. Here we report the results of the search for transient signals from the domain walls of axion-like particles by using the global network of optical magnetometers for exotic (GNOME) physics searches. We search the data, consisting of correlated measurements from optical atomic magnetometers located in laboratories all over the world, for patterns of signals propagating through the network consistent with domain walls. The analysis of these data from a continuous month-long operation of GNOME finds no statistically significant signals, thus placing experimental constraints on such dark matter scenarios.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł

Ta witryna wykorzystuje pliki cookies do przechowywania informacji na Twoim komputerze. Pliki cookies stosujemy w celu świadczenia usług na najwyższym poziomie, w tym w sposób dostosowany do indywidualnych potrzeb. Korzystanie z witryny bez zmiany ustawień dotyczących cookies oznacza, że będą one zamieszczane w Twoim komputerze. W każdym momencie możesz dokonać zmiany ustawień dotyczących cookies