768 results on '"T., Ariga"'
Search Results
2. SMAUG v1.0 – a user-friendly muon simulator for the imaging of geological objects in 3-D
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A. Lechmann, D. Mair, A. Ariga, T. Ariga, A. Ereditato, R. Nishiyama, C. Pistillo, P. Scampoli, M. Vladymyrov, and F. Schlunegger
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Geology ,QE1-996.5 - Abstract
Knowledge about muon tomography has spread in recent years in the geoscientific community and several collaborations between geologists and physicists have been founded. As the data analysis is still mostly done by particle physicists, much of the know-how is concentrated in particle physics and specialised geophysics institutes. SMAUG (Simulation for Muons and their Applications UnderGround), a toolbox consisting of several modules that cover the various aspects of data analysis in a muon tomographic experiment, aims at providing access to a structured data analysis framework. The goal of this contribution is to make muon tomography more accessible to a broader geoscientific audience. In this study, we show how a comprehensive geophysical model can be built from basic physics equations. The emerging uncertainties are dealt with by a probabilistic formulation of the inverse problem, which is finally solved by a Monte Carlo Markov chain algorithm. Finally, we benchmark the SMAUG results against those of a recent study, which, however, have been established with an approach that is not easily accessible to the geoscientific community. We show that they reach identical results with the same level of accuracy and precision.
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- 2022
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3. Vacuum brazing of titanium alloy to stainless steel enhance by fiber laser surface texturing
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A.J. Sulaiman H, M.H. Aiman, M. Ishak, M.M Quazi, T. Zaharinie, and T. Ariga
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vacuum brazing ,titanium alloy ,dissimilar joint ,stainless steel ,geometry surface analysis ,mechanical testing ,Mechanical engineering and machinery ,TJ1-1570 ,Mechanics of engineering. Applied mechanics ,TA349-359 - Abstract
A method for improving the brazing joining strength of Titanium alloy/Stainless steel fabricated through fibre laser surface texturing is introduced because it is a simple process that does not require the fabrication of complicated interlayers. However, previous research shows that a milimeter scale was fabricated by surface modification for dissimilar brazing join, yielding insignificant results and limiting the application and degree of enhancement. Fiber laser ablation was used in this study to create microscale periodic patterns (grooves) on a stainless steel surface. No defect or damage induced during laser surface texturing process. The groove dimension was tunable by controlling the laser parameters. Vacuum brazing of Ti6Al4V to 316L stainless steel with surface texturing, the average joint strength was 22.1 MPa, 34% of increase of joining strength compared to unprocessed flat surface. The combination of laser surface texturing and brazing proven effectively on joining strength enhancement.
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- 2021
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4. OPERA tau neutrino charged current interactions
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N. Agafonova, A. Alexandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievsky, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, S. Gorbunov, Y. Gornushkin, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, K. Ishiguro, A. Iuliano, K. Jakovčić, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Kliček, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Lavasa, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, S. Ogawa, N. Okateva, K. Ozaki, A. Paoloni, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, I. Shakirianova, A. Schembri, T. Shchedrina, E. Shibayama, H. Shibuya, T. Shiraishi, T. Šimko, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipčević, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, I. Tsanaktsidis, S. Tufanli, A. Ustyuzhanin, S. Vasina, M. Vidal García, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, and C. S. Yoon
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Science - Abstract
Measurement(s) tau neutrino Technology Type(s) detector Sample Characteristic - Environment neutrino beam Sample Characteristic - Location Laboratori Nazionali del Gran Sasso Machine-accessible metadata file describing the reported data: https://doi.org/10.6084/m9.figshare.14979858
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- 2021
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5. First observation of a tau neutrino charged current interaction with charm production in the OPERA experiment
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, S. Gorbunov, Y. Gornushkin, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, K. Ishiguro, A. Iuliano, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, N. Okateva, S. Ogawa, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakirianova, T. Shchedrina, H. Shibuya, E. Shibayama, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, and C. S. Yoon
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Astrophysics ,QB460-466 ,Nuclear and particle physics. Atomic energy. Radioactivity ,QC770-798 - Abstract
Abstract An event topology with two secondary vertices compatible with the decay of short-lived particles was found in the analysis of neutrino interactions in the OPERA target. The observed topology is compatible with tau neutrino charged current (CC) interactions with charm production and neutrino neutral current (NC) interactions with $$c\overline{c}$$ cc¯ pair production. However, other processes can mimic this topology. A dedicated analysis was implemented to identify the underlying process. A Monte Carlo simulation was developed and complementary procedures were introduced in the kinematic reconstruction. A multivariate analysis technique was used to achieve an optimal separation of signal from background. Most likely, this event is a $$\nu _{\tau }$$ ντ CC interaction with charm production, the tau and charm particle decaying into 1 prong and 2 prongs, respectively. The significance of this observation is evaluated.
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- 2020
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6. Effect of copper based filler composition on the strength of brazed joint
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A. J. Sulaiman H., W. N. W. M. N. Hissyam, Aiman M. H., M. Ishak, and T. Ariga
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intermetallic compound (imc) ,shear strength ,temperature ,copper-based filler ,Mechanical engineering and machinery ,TJ1-1570 ,Mechanics of engineering. Applied mechanics ,TA349-359 - Abstract
Vacuum brazing of copper-based filler was performed using pure copper plate as its based metal. The brazed joint was obtained at different temperatures, 680oC and 730oC, with same holding time, which is 30 minutes. MBF 2005 (Cu, 5.7wt.%Ni, 9.7wt.%Sn, 7.0wt.%P), MBF 2002 (Cu, 9.9wt.%Ni, 4.0wt.%Sn, 7.8wt.%P) and VZ 2250 (Cu, 7.0wt.%Ni, 9.3wt.%Sn, 6.3wt.%P) alloys were used as brazing filler materials. The intermetallic compound (IMC) and mechanical properties of the joints were investigated in detail. The result show that the interfacial microstructure of the brazed joints is Cu3P and (CuNi)2P. As the brazing temperature increase from 680oC to 730oC, the IMC become thicker leading to decrease in joining strength due to brittle IMC formation. The maximum shear strength reached 112 MPa at 680oC for MBF 2002 and 129 MPa at 730oC for MBF 2005. Hence, it is found that the composition of filler effects the strength of brazed joint.
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- 2019
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7. The effect of rock composition on muon tomography measurements
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A. Lechmann, D. Mair, A. Ariga, T. Ariga, A. Ereditato, R. Nishiyama, C. Pistillo, P. Scampoli, F. Schlunegger, and M. Vladymyrov
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Geology ,QE1-996.5 ,Stratigraphy ,QE640-699 - Abstract
In recent years, the use of radiographic inspection with cosmic-ray muons has spread into multiple research and industrial fields. This technique is based on the high-penetration power of cosmogenic muons. Specifically, it allows the resolution of internal density structures of large-scale geological objects through precise measurements of the muon absorption rate. So far, in many previous works, this muon absorption rate has been considered to depend solely on the density of traversed material (under the assumption of a standard rock) but the variation in chemical composition has not been taken seriously into account. However, from our experience with muon tomography in Alpine environments, we find that this assumption causes a substantial bias in the muon flux calculation, particularly where the target consists of high {Z2∕A} rocks (like basalts and limestones) and where the material thickness exceeds 300 m. In this paper, we derive an energy loss equation for different minerals and we additionally derive a related equation for mineral assemblages that can be used for any rock type on which mineralogical data are available. Thus, for muon tomography experiments in which high {Z2∕A} rock thicknesses can be expected, it is advisable to plan an accompanying geological field campaign to determine a realistic rock model.
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- 2018
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8. A cold/ultracold neutron detector using fine-grained nuclear emulsion with spatial resolution less than 100 nm
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N. Naganawa, T. Ariga, S. Awano, M. Hino, K. Hirota, H. Kawahara, M. Kitaguchi, K. Mishima, H. M. Shimizu, S. Tada, S. Tasaki, and A. Umemoto
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Astrophysics ,QB460-466 ,Nuclear and particle physics. Atomic energy. Radioactivity ,QC770-798 - Abstract
Abstract A new type of cold/ultracold neutron detector that can realize a spatial resolution of less than 100 nm was developed using nuclear emulsion. The detector consists of a fine-grained nuclear emulsion coating and a 50-nm thick $$^{10}\hbox {B}_4 \hbox {C}$$ 10B4C layer for the neutron conversion. The detector was exposed to cold and ultracold neutrons (UCNs) at the J-PARC. Detection efficiencies were measured as (0.163 ± 0.015 (stat) ± 0.013 (sys))% and (10.3 ± 1.3 (stat) ± 1.1 (sys))% for cold and ultracold neutrons consistently with the $$^{10}$$ 10 B content in the converter. Positions of individual neutrons can be determined by observing secondary particle tracks recorded in the nuclear emulsion. The spatial resolution of incident neutrons were found to be in the range of 11–99 nm in the angle region of tan$$\theta \le 1.9$$ θ≤1.9 , where $$\theta $$ θ is the angle between a recorded track and the normal direction of the converter layer. The achieved spatial resolution corresponds to the improvement of one or two orders of magnitude compared with conventional techniques and it is comparable with the wavelength of UCNs.
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- 2018
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9. Final results of the search for ν μ → ν e oscillations with the OPERA detector in the CNGS beam
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The OPERA collaboration, N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievsky, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, J. Favier, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, Y. Gornushkin, S. Gorbunov, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, B. Hosseini, K. Ishiguro, A. Iuliano, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, F. Meisel, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, N. Okateva, S. Ogawa, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, H. Shibuya, E. Shibayama, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, and C. S. Yoon
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Neutrino Detectors and Telescopes (experiments) ,Oscillation ,Nuclear and particle physics. Atomic energy. Radioactivity ,QC770-798 - Abstract
Abstract The OPERA experiment has discovered the tau neutrino appearance in the CNGS muon neutrino beam, in agreement with the 3 neutrino flavour oscillation hypothesis. The OPERA neutrino interaction target, made of Emulsion Cloud Chambers, was particularly efficient in the reconstruction of electromagnetic showers. Moreover, thanks to the very high granularity of the emulsion films, showers induced by electrons can be distinguished from those induced by π 0s, thus allowing the detection of charged current interactions of electron neutrinos. In this paper the results of the search for electron neutrino events using the full dataset are reported. An improved method for the electron neutrino energy estimation is exploited. Data are compatible with the 3 neutrino flavour mixing model expectations and are used to set limits on the oscillation parameters of the 3+1 neutrino mixing model, in which an additional mass eigenstate m 4 is introduced. At high Δm 412 (≳0.1 eV2), an upper limit on sin2 2θ μe is set to 0.021 at 90% C.L. and Δm 412 ≳ 4 × 10− 3 eV2 is excluded for maximal mixing in appearance mode.
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- 2018
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10. Study of charged hadron multiplicities in charged-current neutrino–lead interactions in the OPERA detector
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, I. Bodnarchuk, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, Y. Gornushkin, S. Gorbunov, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, B. Hosseini, K. Ishiguro, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, N. Okateva, S. Ogawa, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakirianova, T. Shchedrina, H. Shibuya, E. Shibayama, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, and C. S. Yoon
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Astrophysics ,QB460-466 ,Nuclear and particle physics. Atomic energy. Radioactivity ,QC770-798 - Abstract
Abstract The OPERA experiment was designed to search for $$\nu _{\mu } \rightarrow \nu _{\tau }$$ νμ→ντ oscillations in appearance mode through the direct observation of tau neutrinos in the CNGS neutrino beam. In this paper, we report a study of the multiplicity of charged particles produced in charged-current neutrino interactions in lead. We present charged hadron average multiplicities, their dispersion and investigate the KNO scaling in different kinematical regions. The results are presented in detail in the form of tables that can be used in the validation of Monte Carlo generators of neutrino–lead interactions.
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- 2018
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11. Metallurgical and shear strength of brazed bulk pure copper by microwave hybrid heating
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Maisarah Lutfi, F. Yusof, S. Ramesh, and T. Ariga
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- 2023
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12. Erratum to: Study of charged hadron multiplicities in charged-current neutrino–lead interactions in the OPERA detector
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, I. Bodnarchuk, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, Y. Gornushkin, S. Gorbunov, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, B. Hosseini, K. Ishiguro, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, N. Okateva, S. Ogawa, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakirianova, T. Shchedrina, H. Shibuya, E. Shibayama, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, and C. S. Yoon
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Astrophysics ,QB460-466 ,Nuclear and particle physics. Atomic energy. Radioactivity ,QC770-798 - Abstract
Section Analysis, line 9: sub-sample of 818 events becomes sub-sample of 817 events.
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- 2018
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13. Multi-Objective Optimization of Mn-Doped Tio2 Content for Wettability, Printability and Intermetallic Layer of Sac305 Pb-Free Solder Paste on a Cu Substrate
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T. Ariga and K. Kanlayasiri
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Surface-mount technology ,Materials science ,Strategy and Management ,Tio2 nanoparticles ,Intermetallic ,Solder paste ,Mn doped ,Substrate (electronics) ,Wetting ,Composite material ,Layer (electronics) ,Industrial and Manufacturing Engineering ,Computer Science Applications - Abstract
Effects of Mn-doped TiO2 nanoparticles on the wettability, printability and thickness of intermetallic layer of SAC30 on a Cu substrate were studied in this paper. Concentration of Mn-doped TiO2 nanoparticles was varied from 0.05 wt.% to 1[Formula: see text]wt.%. The wettability was evaluated in terms of contact angle of solder on the copper substrate and the printability was measured from the volume ratio of printed solder on the copper substrate to volume of stencil opening. The experimental results showed that 0.10[Formula: see text]wt.% Mn-doped TiO2 led to the lowest contact angle while the printability was decreased with the increase of the added nanoparticles and the thinnest intermetallic layer was found at 0.50[Formula: see text]wt.% Mn-doped TiO2 nanoparticles. Mn-doped TiO2 concentration was then optimized using a desirability function to find optimal values for the three responses. It was found that 0.07[Formula: see text]wt.% was the optimal concentration for the three metrics — wettability, printability and thickness of the intermetallic layer.
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- 2021
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14. Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam
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N. Agafonova, A. Alexandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, M. Chernyavskiy, A. Chukanov, L. Consiglio, N. D'Ambrosio, G. De Lellis, M. De Serio, P. del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievsky, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, J. Favier, R. A. Fini, F. Fornari, T. Fukuda, G. Galati, A. Garfagnini, V. Gentile, J. Goldberg, S. Gorbunov, Y. Gornushkin, G. Grella, A. M. Guler, C. Gustavino, C. Hagner, T. Hara, T. Hayakawa, A. Hollnagel, K. Ishiguro, A. Iuliano, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, F. Laudisio, A. Lauria, A. Longhin, P. Loverre, M. Malenica, A. Malgin, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, M. Miyanishi, F. Mizutani, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, K. Niwa, S. Ogawa, A. Olchevsky, N. Okateva, K. Ozaki, A. Paoloni, L. Paparella, B. D. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, T. Roganova, H. Rokujo, G. Rosa, O. Ryazhskaya, A. Sadovsky, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, E. Shibayama, H. Shibuya, T. Shiraishi, S. Simone, C. Sirignano, G. Sirri, A. Sotnikov, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, A. Ustyuzhanin, S. Vasina, P. Vilain, E. Voevodina, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon
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Physics ,QC1-999 - Abstract
OPERA is a long-baseline experiment designed to search for $\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode. It was based at the INFN Gran Sasso laboratory (LNGS) and took data from 2008 to 2012 with the CNGS neutrino beam from CERN. After the discovery of $\nu_\tau$ appearance in 2015, with $5.1\sigma$ significance, the criteria to select $\nu_\tau$ candidates have been extended and a multivariate approach has been used for events identification. In this way the statistical uncertainty in the measurement of the oscillation parameters and of $\nu_\tau$ properties has been improved. Results are reported.
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- 2019
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15. Management Of Postoperative Dysphagia After Esophagectomy For Esophageal Cancer
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Y. Hiramatsu, T. Ariga, T. Nagafusa, J. Honke, R. Haneda, S. Kawata, T. Murakami, E. Booka, T. Matsumoto, Y. Shirai, Y. Morita, H. Kikuchi, A. Kato, K. Yamauchi, and H. Takeuchi
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Nutrition and Dietetics ,Endocrinology, Diabetes and Metabolism - Published
- 2023
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16. Chemical constituents and bioactivity of Piper sarmentosum: a mini review
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T. Ariga, A. Azleen, Zarani Mat Taher, S. Sasano, and A.A. Aziz
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biology ,Traditional medicine ,Chemistry ,Chemical constituents ,Piper sarmentosum ,biology.organism_classification ,complex mixtures ,Food Science ,Mini review - Abstract
Herbs with medicinal potential are important for health and wellness. The main aim of this review article was to disseminate important information regarding the use of Piper sarmentosum as natural medicine. P. sarmentosum have been reported to possess a varying degree of hypoglycemic, antidiabetic and other additional properties. The antioxidant properties of the herbs may be effective in controlling the oxidative damage. The review article highlights the positive role of traditional herbs as alternative medicine.
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- 2020
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17. Characterization of a hamster melanoma-associated ganglioside antigen as 7-O-acetylated disialoganglioside GD3
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S Ren, T Ariga, JN Scarsdale, Y Zhang, A Slominski, PO Livingston, G Ritter, Y Kushi, and RK Yu
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Biochemistry ,QD415-436 - Abstract
We previously reported a hamster animal model of melanoma in which the tumor tissue expresses gangliosides GM3, GD3, and O-acetyl GD3. This ganglioside pattern is similar to that in human melanomas (Ren, S., A. Slominski, and R. K. Yu. 1989 Cancer Res. 49: 7051). In this study, we isolated and purified these gangliosides using chloroform-methanol extraction, Folch partition, chromatographies on DEAE-Sephadex A-25, and Iatrobeads columns. The yields of gangliosides GM3, GD3, and O-acetyl GD3 were 44.1 mg, 19.6 mg, and 9 mg per 100 g of Ma melanotic melanoma tissues, respectively. The structures of these gangliosides were characterized by periodate oxidation, gas chromatographic (GC) analysis, fast-atom bombardment-mass spectrometry (FAB-MS), and nuclear magnetic resonance (NMR) studies. The structure of hamster melanoma O-acetyl GD3 is different from the 9-O-acetyl GD3 previously reported in human melanoma. The major fatty acids of this ganglioside are C16:0, C18:0, C20:0, C22:0, and C24:0 and the long-chain base is C18-sphingosine.
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- 1993
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18. UDP-galactose:globotriaosylceramide alpha-galactosyltransferase activity in rat pheochromocytoma (PC12h) cells.
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S Pal, M Saito, T Ariga, and RK Yu
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Biochemistry ,QD415-436 - Abstract
The activity of alpha-galactosyltransferase in cultured rat pheochromocytoma subcloned (PC12h) cells was examined using Gb3 as the acceptor for the galactose from UDP-galactose. The major reaction product was identified as gal alpha 1-3Gb3 based on its mobility on thin-layer chromatographic (TLC) plates and susceptibility to specific galactosidases. The enzyme activity in PC12h cells was the highest at pH 7.0 while the presence of Triton CF-54 (0.1%) and Mn2+ (5 mM) was required for its full activity. The apparent Km values for Gb3 and UDP-galactose were 57 and 17 microM, respectively. The enzyme activity in PC12h cells was compared with that in parent PC12 cells, in which gal alpha 1-3Gb3 is not expressed in an appreciable amount. In the enzyme reaction with exogenous Gb3, the enzyme activity in PC12h cells was about 1.5-fold higher than that in PC12 cells. In the absence of exogenous Gb3, this difference became even more pronounced; gal alpha 1-3Gb3 was generated from endogenous Gb3 at a much higher rate in PC12h cells than in PC12 cells. These findings suggest that the higher level of the alpha-galactosyltransferase activity in PC12h cells may, at least in part, be responsible for the accumulation of unique neutral glycosphingolipids having gal alpha 1-3 terminal residues in the cells.
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- 1992
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19. Biochemical and clinical analysis of accumulated glycolipids in symptomatic heterozygotes of angiokeratoma corporis diffusum (Fabry's disease) in comparison with hemizygotes.
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I Hozumi, M Nishizawa, T Ariga, and T Miyatake
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Biochemistry ,QD415-436 - Abstract
Angiokeratoma corporis diffusum (Fabry's disease) is an X-linked disorder of glycosphingolipid catabolism. Heterozygous females, although usually asymptomatic, are occasionally as severely afflicted as hemizygous males; recently we identified a heterozygous patient with cardiomyopathy and severe pain in the extremities. In order to elucidate the difference of the clinical features, we analyzed the glycolipid composition of the heart, liver, and kidney obtained from the patient and from a hemizygote. Gas-liquid chromatography revealed that globotriaosylceramide (Gb3) was markedly increased in the heart (32.4 times higher than control) and increased to a lesser extent in the liver and kidney (3.74 and 6.79 times, respectively). The pattern of Gb3 accumulation in the heterozygote, where the highest increases were seen in the heart, was distinct from that in the hemizygote, where elevated levels of Gb3 and Ga2 were found in the kidney. Furthermore, the alpha-galactosidase activity in the heart, liver, and kidney of the heterozygote was 17%, 26%, and 36%, respectively, of normal controls, which correlated well with the accumulation of glycosphingolipid in the heart and with the disease's clinical manifestations. Two other hemizygotic patients, who were identified by low alpha-galactosidase activities, demonstrated the cardiac involvement.
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- 1990
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20. Effect of copper based filler composition on the strength of brazed joint
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T. Ariga, M. Ishak, Aiman M. H., W. N. W. M. N. Hissyam, and A. J. Sulaiman H.
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Materials science ,Mechanical Engineering ,Computational Mechanics ,Intermetallic ,Energy Engineering and Power Technology ,chemistry.chemical_element ,Microstructure ,Copper ,Industrial and Manufacturing Engineering ,Metal ,Fuel Technology ,Brittleness ,chemistry ,Mechanics of Materials ,visual_art ,visual_art.visual_art_medium ,Shear strength ,Brazing ,Composite material ,Joint (geology) - Abstract
Vacuum brazing of copper-based filler was performed using pure copper plate as its based metal. The brazed joint was obtained at different temperatures, 680oC and 730oC, with same holding time, which is 30 minutes. MBF 2005 (Cu, 5.7wt.%Ni, 9.7wt.%Sn, 7.0wt.%P), MBF 2002 (Cu, 9.9wt.%Ni, 4.0wt.%Sn, 7.8wt.%P) and VZ 2250 (Cu, 7.0wt.%Ni, 9.3wt.%Sn, 6.3wt.%P) alloys were used as brazing filler materials. The intermetallic compound (IMC) and mechanical properties of the joints were investigated in detail. The result show that the interfacial microstructure of the brazed joints is Cu3P and (CuNi)2P. As the brazing temperature increase from 680oC to 730oC, the IMC become thicker leading to decrease in joining strength due to brittle IMC formation. The maximum shear strength reached 112 MPa at 680oC for MBF 2002 and 129 MPa at 730oC for MBF 2005. Hence, it is found that the composition of filler effects the strength of brazed joint.
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- 2019
21. Effect of Laser Surface Modification (LSM) on laser energy absorption for laser brazing
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T Ariga, A.Q. Zaifuddin, M. M. Quazi, M. H. Aiman, and Mahadzir Ishak
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Materials science ,Laser scanning ,business.industry ,Oxide ,Laser ,law.invention ,chemistry.chemical_compound ,chemistry ,law ,Surface roughness ,Optoelectronics ,Surface modification ,Focal length ,Brazing ,Laser power scaling ,business - Abstract
Since the development of the laser in the 1960s a rapid development of research interests in science and technology took place. Since then, the need of laser application in industrials such as automotive, aerospace and electronics is increasing because of several advantages like automation worthiness, noncontact processing and product quality improvement. In this present study, the effect of Laser Surface Modification (LSM) on pure copper plate towards the laser energy absorption during indirect laser brazing process was studied. The laser brazing experiment was conducted inside a chamber under controlled vacuum pressure with 400Pa and irradiated with constant 140 Watt laser power. The defocusing features for laser brazing was used in order to find better focal position. Accordingly, the focal length for this laser brazing experiment was set to the focus point at 124 mm from the focal plane. Meanwhile, during LSM process, laser parameters such as laser scanning speed and focus length have been kept constant throughout the surface modification process. Yet, the laser power and laser frequency have been varied from 9 Watt to 27 Watt and 10 kHz to 80 kHz respectively. Apparently, surface roughness due to surface removal and oxide layer formation were presented during LSM process. These two surface integrities were found to be the factors of increasing laser energy absorption. It was discovered that an increase in surface roughness and oxide layer formation can absorb more laser energy which then results an increase in brazing temperature during laser brazing. This is because, increasing surface roughness will scatter the laser energy over a larger surface area, multiply the reflections in the surface irregularities while the oxide layer will enhance the interference phenomena of laser energy occurring inside the oxide layer. Both mechanisms increase laser energy absorptivity during laser brazing which results a high brazing temperature.
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- 2020
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22. Enhancement of mechanical properties of Copper Brazed by laser surface modification
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A J Sulaiman, T Ariga, M. H. Aiman, Mahadzir Ishak, and M. M. Quazi
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Shear (sheet metal) ,Materials science ,Filler metal ,visual_art ,visual_art.visual_art_medium ,Brazing ,Surface modification ,Laser power scaling ,Wetting ,Ceramic ,Composite material ,Tensile testing - Abstract
Nowadays, laser surface modification (LSM) has become the most advance technique for improving the surface properties for joining methods. This is due to its advantages such as cleaner, precise, more reliable and provides exact control compare to other surface modification techniques. This technique also applicable on wide range of materials, such as metal/alloy, ceramic and polymer. Brazing is a metal-joining process in which two or more metal items are joint together by melting and flowing a filler metal into the joint, the filler metal having a lower melting point than the base materials. The brazing process performed under a controlled atmosphere in vacuum tube furnace. Microscopic observations were made by use of both optical and electron microscopes. Fibre laser surface modification-brazing of 2 mm thick 99% pure copper plate in the lap joint configuration performing with Cu-based filler metal. There are three microgrooves were produced with three different laser power apply 15 watt, 21 watt and 27 watt. It found that successful brazing and wetting can be achieved by modified the surface for the base metal. The result of shear tensile test indicated that the highest shear strength was achieve in groove by using 27. This is because of its excellent of its excellent spreading behaviour of molten filler metal, largest bonding interface area and suitable intermetallic compound (IMC) distribution.
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- 2020
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23. Detecting differences with magnetoencephalography (MEG)-urodynamics study of somatosensory processing normal desire to void and maximum desire to void sensation
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T. Kitta, H. Shiraishi, K. Yagyu, A. Shimojo, K. Egawa, Y. Kanno, M. Ouchi, M. Higuchi, M. Togo, Y. Takahashi, M. Tsukiyama, K. Moriya, T. Ariga, and N. Shinohara
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Urology - Published
- 2019
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24. The DUNE Far Detector Interim Design Report Volume 1: Physics, Technology and Strategies
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Collaboration, D, Abi, B, Acciarri, R, Acero, M, Adamowski, M, Adams, C, Adams, D, Adamson, P, Adinolfi, M, Ahmad, Z, Albright, C, Aliaga Soplin, L, Alion, T, Alonso Monsalve, S, Alrashed, M, Alt, C, Anderson, J, Anderson, K, Andreopoulos, C, Andrews, M, Andrews, R, Ankowski, A, Anthony, J, Antonello, M, Antonova, M, Antusch, S, Aranda Fernandez, A, Ariga, A, Ariga, T, Aristizabal Sierra, D, Arrieta Diaz, E, Asaadi, J, Ascencio, M, Asner, D, Athar, M, Auger, M, Aurisano, A, Aushev, V, Autiero, D, Azfar, F, Back, A, Back, H, Back, J, Backhouse, C, Baesso, P, Bagby, L, Bai, X, Baird, M, Balantekin, B, Balasubramanian, S, Baller, B, Ballett, P, Balleyguier, L, Bambah, B, Band, H, Bansal, M, Bansal, S, Barenboim, G, Barker, G, Barnes, C, Barr, G, Barranco Monarca, J, Barros, N, Barrow, J, Bashyal, A, Basque, V, Bass, M, Bay, F, Bays, K, Bazo, J, Beacom, J, Bechetoille, E, Behera, B, Bellantoni, L, Bellettini, G, Bellini, V, Beltramello, O, Belver, D, Benekos, N, Benetti, P, Bercellie, A, Berman, E, Bernardini, P, Berner, R, Berns, H, Bernstein, R, Bertolucci, S, Betancourt, M, Bhatnagar, V, Bhattacharjee, M, Bhuyan, B, Biagi, S, Bian, J, Biery, K, Bilki, B, Bishai, M, Bitadze, A, Blackburn, T, Blake, A, Blanco Siffert, B, Blaszczyk, F, Blaufuss, E, Blazey, G, Blennow, M, Blucher, E, Bocean, V, Boffelli, F, Boissevain, J, Bolognesi, S, Bolton, T, Bonesini, M, Boone, T, Booth, A, Booth, C, Bordoni, S, Borkum, A, Boschi, T, Bour, P, Bourguille, B, Boyd, S, Boyden, D, Bracinik, J, Brailsford, D, Brandt, A, Bremer, J, Brice, S, Bromberg, C, Brooijmans, G, Brooke, J, Brown, G, Buchanan, N, Budd, H, de Holanda, P, Cai, T, Caiulo, D, Calafiura, P, Calatayud, A, Calcutt, J, Callahan, C, Calligarich, E, Calvo, E, Camilleri, L, Caminata, A, Campanelli, M, Cancelo, G, Cankocak, K, Cantini, C, Caratelli, D, Carlus, B, Carneiro, M, Caro Terrazas, I, Carroll, T, Carvallo, M, Cascella, M, Castromonte, C, Catano-Mur, E, Cavalli-Sforza, M, Cavanna, F, Cazzato, E, Centro, S, Cerati, G, Cervelli, A, Cervera Villanueva, A, Cervi, T, Chalifour, M, Chappuis, A, Chatterjee, A, Chattopadhyay, S, Chaves, J, Chen, H, Chen, M, Chen, S, Cherdack, D, Chi, C, Childress, S, Cho, K, Choubey, S, Choudhary, B, Christensen, A, Christian, D, Christodoulou, G, Christofferson, C, Church, E, Clarke, P, Coan, T, Cocco, A, Collin, G, Conley, E, Conrad, J, Convery, M, Corey, R, Corwin, L, Cotte, P, Cremonesi, L, Crespo-Anadón, J, Creus Prats, J, Cristaldo, E, Crivelli, P, Cronin-Hennessy, D, Crowley, C, Cuesta, C, Curioni, A, Cussans, D, Dabrowski, M, Dale, D, Da Motta, H, Davenne, T, Davenport, E, Davies, G, Davies, J, Davini, S, Dawson, J, De, K, Decowski, M, Dedin Neto, P, de Icaza Astiz, I, Delbart, A, Delepine, D, Delgado, M, Dell, A, de Mello Neto, J, Demuth, D, Deng, Z, Dennis, S, Densham, C, De Bonis, I, De Gouvêa, A, De Jong, P, De Lurgio, P, De Rijck, S, De Roeck, A, de Vries, J, Dharmapalan, R, Dhingra, N, Diamantopoulou, M, Diaz, F, Díaz, J, Diaz Bautista, G, Ding, P, Distefano, C, Diwan, M, Di Domizio, S, Di Giulio, L, Di Luise, S, Djurcic, Z, Doizon, F, Dokania, N, Dolinski, M, Dong, R, dos Anjos, J, Douglas, D, Drake, G, Duchesneau, D, Duffy, K, Dung, B, Dutta, D, Duvernois, M, Duyang, H, Dvornikov, O, Dwyer, D, Dye, S, Dyshkant, A, Dytman, S, Eads, M, Eberly, B, Edmunds, D, Eisch, J, Elagin, A, Elliott, S, Ellsworth, W, Elnimr, M, Emery, S, Eno, S, Ereditato, A, Escobar, C, Escudero Sanchez, L, Evans, J, Ezeribe, A, Fahey, K, Falcone, A, Falk, L, Farbin, A, Farnese, C, Farzan, Y, Fasoli, M, Fava, A, Felix, J, Fernandez-Martinez, E, Fernandez Menendez, P, Ferraro, F, Feyzi, F, Fields, L, Filkins, A, Filthaut, F, Finch, A, Fischer, O, Fitton, M, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Forest, T, Fowler, J, Fox, W, Franc, J, Francis, K, Franchini, P, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gago, A, Gallagher, H, Gallego-Ros, A, Galymov, V, Gamberini, E, Gambetta, S, Gamble, T, Gandhi, R, Gandrajula, R, Gao, S, Garcia-Gamez, D, Gardiner, S, Gastler, D, Gehrlein, J, Gelli, B, Gendotti, A, Ghorbani-Moghaddam, Z, Ghosh, A, Gibin, D, Gil-Botella, I, Girerd, C, Giri, A, Glavin, S, Goeldi, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Gomez, L, Gomez Bermeo, L, Gomez Cadenas, J, Gong, H, Gonnella, F, Gonzalez-Cuevas, J, Goodman, M, Goodwin, O, Gorbunov, D, Goswami, S, Goudzovski, E, Grace, C, Graf, N, Graham, M, Gramellini, E, Gran, R, Grant, A, Grant, C, Grant, N, Greco, V, Green, S, Greenlee, H, Greenler, L, Greenwood, M, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Guanghua, G, Guardincerri, E, Guarino, V, Guedes, G, Guenette, R, Guglielmi, A, Guo, B, Gupta, S, Gupta, V, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Habig, A, Hackenburg, R, Hackenburg, A, Hackett, B, Hadavand, H, Haenni, R, Hahn, A, Haigh, J, Haines, T, Haiston, J, Hamernik, T, Hamilton, P, Han, J, Handler, T, Hans, S, Harris, D, Hartnell, J, Hasegawa, T, Hatcher, R, Hatzikoutelis, A, Hays, S, Hazen, E, Headley, M, Heavey, A, Heegerv, K, Heise, J, Hennessy, K, Henry, S, Hernandez, A, Hernandez-Garcia, J, Herner, K, Hewes, J, Hignight, J, Higuera, A, Hill, T, Hillier, S, Himmel, A, Hohl, C, Holin, A, Hoppe, E, Horikawa, S, Horton-Smith, G, Hostert, M, Hourlier, A, Howard, B, Howell, R, Huang, J, Hugon, J, Hurh, P, Hylen, J, Illingworth, R, Insler, J, Introzzi, G, Ioannisian, A, Izmaylov, A, Jaffe, D, James, C, James, E, Jang, C, Jediny, F, Jeong, Y, Jhingan, A, Ji, W, Jipa, A, Jiménez, S, Johnson, C, Johnson, M, Johnson, R, Johnstone, J, Jones, B, Jones, S, Joshi, J, Jostlein, H, Jung, C, Junk, T, Kaboth, A, Kadenko, I, Kamiya, F, Kamyshkov, Y, Karagiorgi, G, Karasavvas, D, Karyotakis, Y, Kasai, S, Kasetti, S, Kaur, K, Kayser, B, Kazaryan, N, Kearns, E, Keener, P, Kemp, E, Kendziora, C, Ketchum, W, Kettell, S, Khabibullin, M, Khotjantsev, A, Kim, D, Kirby, B, Kirby, M, Klein, J, Ko, Y, Kobilarcik, T, Kocaman, B, Koerner, L, Kohn, S, Koizumi, G, Koller, P, Kopylov, A, Kordosky, M, Kormos, L, Kosc, T, Kose, U, Kostelecký, V, Kothekar, K, Kramer, M, Krennrich, F, Kreslo, I, Kriesel, K, Kropp, W, Kudenko, Y, Kudryavtsev, V, Kulagin, S, Kumar, J, Kumar, L, Kumar, A, Kumbhare, S, Kuruppu, C, Kus, V, Kutter, T, Lazur, R, Lande, K, Lane, C, Lang, K, Langford, T, Lanni, F, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Lazanu, I, Le, T, Learned, J, Lebrun, P, Lee, D, Lehmann Miotto, G, Leigui de Oliveira, M, Li, Q, Li, S, Li, X, Li, Y, Li, Z, Liao, H, Lin, S, Lin, C, Linehan, R, Linhart, V, Link, J, Liptak, Z, Lissauer, D, Littenberg, L, Littlejohn, B, Liu, J, Liu, T, Lomonaco, L, Losecco, J, Lockwitz, S, Lockyer, N, Loew, T, Lokajicek, M, Long, K, Loo, K, Lopez, J, Lorca, D, Lord, T, Losada, M, Louis, W, Luethi, M, Luk, K, Lundin, T, Luo, X, Lurkin, N, Lux, T, Luzio, V, Lykken, J, Maalampi, J, Maclellan, R, Machado, A, Machado, P, Macias, C, Macier, J, Madigan, P, Magill, S, Mahler, G, Mahn, K, Malek, M, Maloney, J, Mammoliti, F, Mandal, S, Mandrioli, G, Manenti, L, Manly, S, Mann, A, Marchionni, A, Marciano, W, Marcocci, S, Marfatia, D, Mariani, C, Maricic, J, Marinho, F, Marino, A, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, D, Martinez, N, Martinez, H, Mason, K, Mastbaum, A, Masud, M, Mathez, H, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mazza, R, Mazzacane, A, Mazzucato, E, Mccauley, N, Mccluskey, E, Mcconkey, N, Mcdonald, K, Mcfarland, K, Mcgivern, C, Mcgowan, A, Mcgrew, C, Mckeown, R, Mcnab, A, Mcnulty, D, Mctaggart, R, Meddage, V, Mefodiev, A, Mehta, P, Mei, D, Mena, O, Menary, S, Mendez, H, Mendez, D, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mewes, M, Meyer, H, Miao, T, Migenda, J, Milincic, R, Miller, J, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Mishra, C, Mishra, S, Mislivec, A, Mitrica, B, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mokhov, N, Molina, J, Molina Bueno, L, Montanari, A, Montanari, C, Montanari, D, 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White, L. H. Whitehead, D. Whittington, K. Wierman, M. Wilking, C. Wilkinson, J. Willhite, Z. Williams, R. J. Wilson, P. Wilson, P. Wittich, J. Wolcott, T. Wongjirad, K. Wood, L. Wood, E. Worcester, M. Worcester, S. Wu, W. Wu, W. Xu, C. Yanagisawa, S. Yang, T. Yang, G. Yang, J. Ye, M. Yeh, N. Yershov, K. Yonehara, L. Yoshimura, B. Yu, J. Yu, J. Zalesak, L. Zambelli, B. Zamorano, A. Zani, K. Zaremba, L. Zazueta, G. P. Zeller, J. Zennamo, C. Zhang, M. Zhao, Y. -L. Zhou, G. Zhu, E. D. Zimmerman, M. Zito, S. Zucchelli, J. Zuklin, V. Zutshi, and R. Zwaska
- Abstract
The DUNE IDR describes the proposed physics program and technical designs of the DUNE Far Detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate milestone on the path to a full TDR, justifying the technical choices that flow down from the high-level physics goals through requirements at all levels of the Project. These design choices will enable the DUNE experiment to make the ground-breaking discoveries that will help to answer fundamental physics questions. Volume 1 contains an executive summary that describes the general aims of this document. The remainder of this first volume provides a more detailed description of the DUNE physics program that drives the choice of detector technologies. It also includes concise outlines of two overarching systems that have not yet evolved to consortium structures: computing and calibration. Volumes 2 and 3 of this IDR describe, for the single-phase and dual-phase technologies, respectively, each detector module's subsystems, the technical coordination required for its design, construction, installation, and integration, and its organizational structure.
- Published
- 2018
25. Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays
- Author
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, B. Büttner, M. Chernyavsky, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. Del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, T. Fukuda, G. Galati, A. Garfagnini, G. Giacomelli, C. Göllnitz, J. Goldberg, Y. Gornushkin, G. Grella, M. Guler, C. Gustavino, C. Hagner, T. Hara, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, J. Kawada, J. H. Kim, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, H. Rokujo, T. Roganova, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, S. Zemskova, A. Zghiche, OpenMETU, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), OPERA, N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, B. Buettner, M. Chernyavsky, A. Chukanov, L. Consiglio, N. D'Ambrosio, G. D. Lelli, M. D. Serio, P. D. Amo, A. D. Crescenzo, D. D. Ferdinando, N. D. Marco, S. Dmitrievski, M. Draco, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, T. Fukuda, G. Galati, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, M. Guler, C. Gustavino, C. Hagner, T. Hara, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, J. Kawada, J. H. Kim, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, H. Rokujo, T. Roganova, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strau, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, S. Zemskova, A. Zghiche, Agafonova, N, Aleksandrov, A, Anokhina, A, Aoki, S, Ariga, A, Ariga, T, Bender, D, Bertolin, A, Bozza, C, Brugnera, R, Buonaura, A, Buontempo, S, Büttner, B, Chernyavsky, M, Chukanov, A, Consiglio, L, D’Ambrosio, N, De Lellis, G, De Serio, M, Del Amo Sanchez, P, Di Crescenzo, A, Di Ferdinando, D, Di Marco, N, Dmitrievski, S, Dracos, M, Duchesneau, D, Dusini, S, Dzhatdoev, T, Ebert, J, Ereditato, A, Fini, R, Fukuda, T, Galati, G, Garfagnini, A, Giacomelli, G, Göllnitz, C, Goldberg, J, Gornushkin, Y, Grella, G, Guler, M, Gustavino, C, Hagner, C, Hara, T, Hollnagel, A, Hosseini, B, Ishida, H, Ishiguro, K, Jakovcic, K, Jollet, C, Kamiscioglu, C, Kamiscioglu, M, Kawada, J, Kim, J, Kim, S, Kitagawa, N, Klicek, B, Kodama, K, Komatsu, M, Kose, U, Kreslo, I, Lauria, A, Lenkeit, J, Ljubicic, A, Longhin, A, Loverre, P, Malgin, A, Malenica, M, Mandrioli, G, Matsuo, T, Matveev, V, Mauri, N, Medinaceli, E, Meregaglia, A, Mikado, S, Monacelli, P, Montesi, M, Morishima, K, Muciaccia, M, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Nakatsuka, Y, Niwa, K, Ogawa, S, Okateva, N, Olshevsky, A, Omura, T, Ozaki, K, Paoloni, A, Park, B, Park, I, Pasqualini, L, Pastore, A, Patrizii, L, Pessard, H, Pistillo, C, Podgrudkov, D, Polukhina, N, Pozzato, M, Pupilli, F, Roda, M, Rokujo, H, Roganova, T, Rosa, G, Ryazhskaya, O, Sato, O, Schembri, A, Shakiryanova, I, Shchedrina, T, Sheshukov, A, Shibuya, H, Shiraishi, T, Shoziyoev, G, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Spinetti, M, Stanco, L, Starkov, N, Stellacci, S, Stipcevic, M, Strauss, T, Strolin, P, Takahashi, S, Tenti, M, Terranova, F, Tioukov, V, Tufanli, S, Vilain, P, Vladimirov, M, Votano, L, Vuilleumier, J, Wilquet, G, Wonsak, B, Yoon, C, Zemskova, S, Zghiche, A, N., Agafonova, Aleksandrov, A., A., Anokhina, S., Aoki, A., Ariga, T., Ariga, D., Bender, A., Bertolin, C., Bozza, R., Brugnera, Buonaura, Annarita, S., Buontempo, B., B?ttner, M., Chernyavsky, A., Chukanov, L., Consiglio, N., D?ambrosio, DE LELLIS, Giovanni, M., De Serio, P., Del Amo Sanchez, DI CRESCENZO, Antonia, D., Di Ferdinando, N., Di Marco, S., Dmitrievski, M., Draco, D., Duchesneau, S., Dusini, T., Dzhatdoev, J., Ebert, A., Ereditato, R. A., Fini, T., Fukuda, Galati, Giuliana, A., Garfagnini, G., Giacomelli, C., G?llnitz, J., Goldberg, Y., Gornushkin, G., Grella, M., Guler, C., Gustavino, C., Hagner, T., Hara, A., Hollnagel, Hosseini, Behzad, H., Ishida, K., Ishiguro, K., Jakovcic, C., Jollet, C., Kamiscioglu, M., Kamiscioglu, J., Kawada, J. H., Kim, S. H., Kim, N., Kitagawa, B., Klicek, K., Kodama, M., Komatsu, U., Kose, I., Kreslo, Lauria, Adele, J., Lenkeit, A., Ljubicic, A., Longhin, P., Loverre, A., Malgin, M., Malenica, G., Mandrioli, T., Matsuo, V., Matveev, N., Mauri, E., Medinaceli, A., Meregaglia, S., Mikado, P., Monacelli, Montesi, MARIA CRISTINA, K., Morishima, M. T., Muciaccia, N., Naganawa, T., Naka, M., Nakamura, T., Nakano, Y., Nakatsuka, K., Niwa, S., Ogawa, N., Okateva, A., Olshevsky, T., Omura, K., Ozaki, A., Paoloni, B. D., Park, I. G., Park, L., Pasqualini, A., Pastore, L., Patrizii, H., Pessard, C., Pistillo, D., Podgrudkov, N., Polukhina, M., Pozzato, F., Pupilli, M., Roda, H., Rokujo, T., Roganova, G., Rosa, O., Ryazhskaya, O., Sato, A., Schembri, I., Shakiryanova, T., Shchedrina, A., Sheshukov, H., Shibuya, T., Shiraishi, G., Shoziyoev, S., Simone, M., Sioli, C., Sirignano, G., Sirri, M., Spinetti, L., Stanco, N., Starkov, S. M., Stellacci, M., Stipcevic, T., Strau, Strolin, PAOLO EMILIO, S., Takahashi, M., Tenti, F., Terranova, V., Tioukov, S., Tufanli, P., Vilain, M., Vladimirov, L., Votano, J. L., Vuilleumier, G., Wilquet, B., Wonsak, C. S., Yoon, S., Zemskova, A., Zghiche, DIP. DI FISICA, DIPARTIMENTO DI FISICA E ASTRONOMIA 'AUGUSTO RIGHI', AREA MIN. 02 - Scienze fisiche, and Da definire
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Particle physics ,Physics and Astronomy (miscellaneous) ,530 Physics ,Hadron ,FOS: Physical sciences ,tau-neutrino interactions ,01 natural sciences ,High Energy Physics - Experiment ,decay ,High Energy Physics - Experiment (hep-ex) ,neutrino ,short-lived particle ,OPERA ,0103 physical sciences ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,Charm (quantum number) ,010306 general physics ,Engineering (miscellaneous) ,Charged current ,neutrino oscillations ,tau neutrino interactions ,emulsion ,Physics ,Interaction point ,010308 nuclear & particles physics ,Emulsion ,0%22">CHARMED MESONS (|C|>0 ,NEUTRINO DETECTORS ,NUCLEAR EMULSION ,chorus experiment ,oscillation ,High Energy Physics::Phenomenology ,Order (ring theory) ,Physique des particules élémentaires ,Particle ,High Energy Physics::Experiment ,Neutrino ,Particle Physics - Experiment ,Lepton - Abstract
The OPERA experiment, designed to perform the first observation of (Formula Presented) oscillations in appearance mode through the detection of the τ leptons produced in ντ charged current interactions, has collected data from 2008 to 2012. In the present paper, the procedure developed to detect τ 1~ from the neutrino interaction point, is described in detail and applied to the search for charmed hadrons, showing similar decay topologies as the τ lepton. In the analysed sample, 50 charm decay candidate events are observed while 54 ±4 are expected, proving that the detector performance and the analysis chain applied to neutrino events are well reproduced by the OPERA simulation and thus validating the methods for ντ appearance detection., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
- Published
- 2014
- Full Text
- View/download PDF
26. Evidence for nu(mu) -> nu(tau) appearance in the CNGS neutrino beam with the OPERA experiment
- Author
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. Ben Dhahbi, A. Badertscher, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, F. Brunet, G. Brunetti, A. Buonaura, S. Buontempo, B. B?ttner, L. Chaussard, M. Chernyavsky, V. Chiarella, A. Chukanov, L. Consiglio, N. D?Ambrosio, M. De Serio, P. Del Amo Sanchez, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, J. Favier, T. Ferber, G. Ferone, R. ?.A. Fini, T. Fukuda, G. Galati, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, M. Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, J. Kawada, H. Kawahara, J. ?.H. Kim, S. ?.H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, P. Migliozzi, S. Mikado, M. Miyanishi, E. Miyashita, P. Monacelli, K. Morishima, M. ?.T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. ?.D. Park, I. ?.G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, H. Rokujo, T. Roganova, G. Rosa, I. Rostovtseva, A. Rubbia, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt Parzefal, I. Shakiryanova, T. Shchedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. ?.M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, K. Suzuki, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. ?.L. Vuilleumier, G. Wilquet, B. Wonsak, C. ?.S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche, DE LELLIS, GIOVANNI, DI CRESCENZO, ANTONIA, LAURIA, ADELE, MONTESI, MARIA CRISTINA, N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. B. Dhahbi, A. Badertscher, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, F. Brunet, G. Brunetti, A. Buonaura, S. Buontempo, B. Buettner, L. Chaussard, M. Chernyavsky, V. Chiarella, A. Chukanov, L. Consiglio, N. D'Ambrosio, G. D. Lelli, M. D. Serio, P. D. Amo, A. D. Crescenzo, D. D. Ferdinando, N. D. Marco, S. Dmitrievski, M. Draco, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, J. Favier, T. Ferber, G. Ferone, R. A. Fini, T. Fukuda, G. Galati, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, M. Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, J. Kawada, H. Kawahara, J. H. Kim, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, P. Migliozzi, S. Mikado, M. Miyanishi, E. Miyashita, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, H. Rokujo, T. Roganova, G. Rosa, I. Rostovtseva, A. Rubbia, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt-Parzefal, I. Shakiryanova, T. Shchedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strau, P. Strolin, K. Suzuki, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche, N., Agafonova, Aleksandrov, A., A., Anokhina, S., Aoki, A., Ariga, T., Ariga, T., Asada, D., Autiero, A., Ben Dhahbi, A., Badertscher, D., Bender, A., Bertolin, C., Bozza, R., Brugnera, F., Brunet, G., Brunetti, A., Buonaura, S., Buontempo, B., B?ttner, L., Chaussard, M., Chernyavsky, V., Chiarella, A., Chukanov, L., Consiglio, N., D?ambrosio, DE LELLIS, Giovanni, M., De Serio, P., Del Amo Sanchez, DI CRESCENZO, Antonia, D., Di Ferdinando, N., Di Marco, S., Dmitrievski, M., Draco, D., Duchesneau, S., Dusini, T., Dzhatdoev, J., Ebert, A., Ereditato, J., Favier, T., Ferber, G., Ferone, Fini, R. ?. A., T., Fukuda, G., Galati, A., Garfagnini, G., Giacomelli, C., Goellnitz, J., Goldberg, Y., Gornushkin, G., Grella, F., Grianti, M., Guler, C., Gustavino, C., Hagner, K., Hakamata, T., Hara, T., Hayakawa, M., Hierholzer, A., Hollnagel, B., Hosseini, H., Ishida, K., Ishiguro, M., Ishikawa, K., Jakovcic, C., Jollet, C., Kamiscioglu, M., Kamiscioglu, T., Katsuragawa, J., Kawada, H., Kawahara, Kim, J. ?. H., Kim, S. ?. H., M., Kimura, N., Kitagawa, B., Klicek, K., Kodama, M., Komatsu, U., Kose, I., Kreslo, Lauria, Adele, J., Lenkeit, A., Ljubicic, A., Longhin, P., Loverre, A., Malgin, G., Mandrioli, J., Marteau, T., Matsuo, V., Matveev, N., Mauri, E., Medinaceli, A., Meregaglia, P., Migliozzi, S., Mikado, M., Miyanishi, E., Miyashita, P., Monacelli, Montesi, MARIA CRISTINA, K., Morishima, Muciaccia, M. ?. T., N., Naganawa, T., Naka, M., Nakamura, T., Nakano, Y., Nakatsuka, K., Niwa, S., Ogawa, N., Okateva, A., Olshevsky, T., Omura, K., Ozaki, A., Paoloni, Park, B. ?. D., Park, I. ?. G., A., Pastore, L., Patrizii, E., Pennacchio, H., Pessard, C., Pistillo, D., Podgrudkov, N., Polukhina, M., Pozzato, K., Pretzl, F., Pupilli, R., Rescigno, M., Roda, H., Rokujo, T., Roganova, G., Rosa, I., Rostovtseva, A., Rubbia, O., Ryazhskaya, O., Sato, Y., Sato, A., Schembri, W., Schmidt Parzefal, I., Shakiryanova, T., Shchedrina, A., Sheshukov, H., Shibuya, T., Shiraishi, G., Shoziyoev, S., Simone, M., Sioli, C., Sirignano, G., Sirri, M., Spinetti, L., Stanco, N., Starkov, Stellacci, S. ?. M., M., Stipcevic, T., Strau, P., Strolin, K., Suzuki, S., Takahashi, M., Tenti, F., Terranova, V., Tioukov, S., Tufanli, P., Vilain, M., Vladimirov, L., Votano, Vuilleumier, J. ?. L., G., Wilquet, B., Wonsak, Yoon, C. ?. S., J., Yoshida, M., Yoshimoto, Y., Zaitsev, S., Zemskova, and A., Zghiche
- Subjects
NEUTRINO OSCILLATIONS ,Physics::Instrumentation and Detectors ,PARTICLE PHYSICS ,oscillation ,neutrino detectors and telescopes ,High Energy Physics::Experiment ,NEUTRINO DETECTORS ,NUCLEAR EMULSION ,TAU LEPTON - Abstract
The OPERA experiment is designed to search for nu(mu) -> nu(tau) oscillations in appearance mode, i.e., through the direct observation of the tau lepton in nu(tau)- charged current interactions. The experiment has taken data for five years, since 2008, with the CERN Neutrino to Gran Sasso beam. Previously, two nu(tau) candidates with a tau decaying into hadrons were observed in a subsample of data of the 2008-2011 runs. Here we report the observation of a third nu(tau) candidate in the tau(-) -> mu(-) decay channel coming from the analysis of a subsample of the 2012 run. Taking into account the estimated background, the absence of nu(mu) -> nu(tau) oscillations is excluded at the 3.4 sigma level.
- Published
- 2014
27. Development of nuclear emulsions with spatial resolution for the AEgIS experiment
- Author
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M. Kimura, S. Aghion, O. Ahl?n, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, G. Bonomi, P. Br?unig, J. Bremer, R. S. Brusa, G. Burghart, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Haider, S. D. Hogan, T. Huse, E. Jordan, L. V. J?rgensen, T. Kaltenbacher, J. Kawada, A. Kellerbauer, A. Knecht, D. Krasnick?, V. Lagomarsino, S. Mariazzi, V. A. Matveev, F. Merkt, F. Moia, G. Nebbia, P. N?d?lec, M. K. Oberthaler, N. Pacifico, V. Petr??ek, C. Pistillo, F. Prelz, M. Prevedelli, C. Regenfus, C. Riccardi, O. R?hne, A. Rotondi, H. Sandaker, J. Storey, M. A. Subieta Vasquez, M. ?pa?ek, G. Testera, D. Trezzi, R. Vaccarone, S. Zavatarelli, SCAMPOLI, PAOLA, M. Kimura, S. Aghion, O. Ahlén, C. Amsler, A. Ariga, T. Ariga, A.S. Belov, G. Bonomi, P. Bräunig, J. Bremer, R.S. Brusa, G. Burghart, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S.N. Gninenko, S. Haider, S.D. Hogan, T. Huse, E. Jordan, L.V. Jørgensen, T. Kaltenbacher, J. Kawada, A. Kellerbauer, A. Knecht, D. Krasnický, V. Lagomarsino, S. Mariazzi, V.A. Matveev, F. Merkt, F. Moia, G. Nebbia, P. Nédélec, M.K. Oberthaler, N. Pacifico, V. Petráček, C. Pistillo, F. Prelz, M. Prevedelli, C. Regenfu, C. Riccardi, O. Røhne, A. Rotondi, H. Sandaker, P. Scampoli, J. Storey, M.A. Subieta Vasquez, M. Špaček, G. Testera, D. Trezzi, R. Vaccarone, S. Zavatarelli, M., Kimura, S., Aghion, O., Ahl?n, C., Amsler, A., Ariga, T., Ariga, A. S., Belov, G., Bonomi, P., Br?unig, J., Bremer, R. S., Brusa, G., Burghart, L., Cabaret, C., Canali, R., Caravita, F., Castelli, G., Cerchiari, S., Cialdi, D., Comparat, G., Consolati, S., Di Domizio, L., Di Noto, M., Doser, A., Dudarev, A., Ereditato, R., Ferragut, A., Fontana, P., Genova, M., Giammarchi, A., Gligorova, S. N., Gninenko, S., Haider, S. D., Hogan, T., Huse, E., Jordan, L. V., J?rgensen, T., Kaltenbacher, J., Kawada, A., Kellerbauer, A., Knecht, D., Krasnick?, V., Lagomarsino, S., Mariazzi, V. A., Matveev, F., Merkt, F., Moia, G., Nebbia, P., N?d?lec, M. K., Oberthaler, N., Pacifico, V., Petr??ek, C., Pistillo, F., Prelz, M., Prevedelli, C., Regenfu, C., Riccardi, O., R?hne, A., Rotondi, H., Sandaker, Scampoli, Paola, J., Storey, M. A., Subieta Vasquez, M., ?pa?ek, G., Testera, D., Trezzi, R., Vaccarone, and S., Zavatarelli
- Subjects
Physics::Instrumentation and Detectors ,ELEMENTARY PARTICLE PHYSICS ,GRAVITATION ,Nuclear Experiment - Abstract
The main goal of the AEgIS experiment at CERN is to test the weak equivalence principle for antimatter. We will measure the Earth's gravitational acceleration g with antihydrogen atoms being launched in a horizontal vacuum tube and traversing a moiré deflectometer. We intend to use a position sensitive device made of nuclear emulsions (combined with a time-of-flight detector such as silicon μ-strips) to measure precisely their annihilation points at the end of the tube. The goal is to determine g with a 1% relative accuracy. In 2012 we tested emulsion films in vacuum and at room temperature with low energy antiprotons from the CERN antiproton decelerator. First results on the expected performance for AEgIS are presented.
- Published
- 2013
28. AEgIS Experiment: Measuring the acceleration g of the earth’s gravitational field on antihydrogen beam
- Author
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L. Bravina, M. A. Subieta Vasquez, S. Aghion, O. Ahlén, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, G. Bonomi, P. Bräunig, J. Bremer, R. S. Brusa, L. Cabaret, M. Caccia, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, L. Dassa, J. H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Heider, S. D. Hogan, T. Huse, E. Jordan, L. V. Jørgensen, T. Kaltenbacher, J. Kawada, A. Kellerbauer, M. Kimura, A. Knecht, D. Krasnický, V. Lagomarsino, S. Mariazzi, V. A. Matveev, F. Merkt, F. Moia, G. Nebbia, P. Nédélec, M. K. Oberthaler, N. Pacifico, V. Petráček, C. Pistilo, F. Prelz, M. Prevedelli, C. Regenfus, C. Ricardi, O. Røhne, A. Rotondi, H. Sandaker, J. Storey, M. Špaček, G. Testera, D. Trezzi, R. Vaccarone, F. Villa, S. Zavatarelli, Y. Foka, S. Kabana, SCAMPOLI, PAOLA, L., Bravina, M. A., Subieta Vasquez, S., Aghion, O., Ahlén, C., Amsler, A., Ariga, T., Ariga, A. S., Belov, G., Bonomi, P., Bräunig, J., Bremer, R. S., Brusa, L., Cabaret, M., Caccia, C., Canali, R., Caravita, F., Castelli, G., Cerchiari, S., Cialdi, D., Comparat, G., Consolati, L., Dassa, J. H., Derking, S., Di Domizio, L., Di Noto, M., Doser, A., Dudarev, A., Ereditato, R., Ferragut, A., Fontana, P., Genova, M., Giammarchi, A., Gligorova, S. N., Gninenko, S., Heider, S. D., Hogan, T., Huse, E., Jordan, L. V., Jørgensen, T., Kaltenbacher, J., Kawada, A., Kellerbauer, M., Kimura, A., Knecht, D., Krasnický, V., Lagomarsino, S., Mariazzi, V. A., Matveev, F., Merkt, F., Moia, G., Nebbia, P., Nédélec, M. K., Oberthaler, N., Pacifico, V., Petráček, C., Pistilo, F., Prelz, M., Prevedelli, C., Regenfu, C., Ricardi, O., Røhne, A., Rotondi, H., Sandaker, Scampoli, Paola, J., Storey, M., Špaček, G., Testera, D., Trezzi, R., Vaccarone, F., Villa, S., Zavatarelli, Y., Foka, and S., Kabana
- Published
- 2014
29. Measuring g with Aegis, Progress and Perspectives
- Author
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D. Krasnick?, S. Aghion, O. Ahl?n, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, K. Berggren, G. Bonomi, P. Br?unig, J. Bremer, R. S. Brusa, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Haider, T. Huse, E. Jordan, L. V. J?rgensen, T. Kaltenbacher, J. Kawada, A. Kellerbauer, M. Kimura, A. Knecht, V. Lagomarsino, S. Lehner, A. Magnani, C. Malbrunot, S. Mariazzi, V. A. Matveev, G. Nebbia, P. N?d?lec, M. K. Oberthaler, N. Pacifico, V. Petr??ek, C. Pistillo, F. Prelz, M. Prevedelli, C. Regenfus, C. Riccardi, O. R?hne, A. Rotondi, H. Sandaker, J. Storey, M. A. Subieta Vasquez, M. ?pa?ek, G. Testera, E. Widmann, P. Yzombard, S. Zavatarelli, J. Zmeskal, SCAMPOLI, PAOLA, D., Krasnick?, S., Aghion, O., Ahl?n, C., Amsler, A., Ariga, T., Ariga, A. S., Belov, K., Berggren, G., Bonomi, P., Br?unig, J., Bremer, R. S., Brusa, L., Cabaret, C., Canali, R., Caravita, F., Castelli, G., Cerchiari, S., Cialdi, D., Comparat, G., Consolati, H., Derking, S., Di Domizio, L., Di Noto, M., Doser, A., Dudarev, A., Ereditato, R., Ferragut, A., Fontana, P., Genova, M., Giammarchi, A., Gligorova, S. N., Gninenko, S., Haider, T., Huse, E., Jordan, L. V., J?rgensen, T., Kaltenbacher, J., Kawada, A., Kellerbauer, M., Kimura, A., Knecht, V., Lagomarsino, S., Lehner, A., Magnani, C., Malbrunot, S., Mariazzi, V. A., Matveev, G., Nebbia, P., N?d?lec, M. K., Oberthaler, N., Pacifico, V., Petr??ek, C., Pistillo, F., Prelz, M., Prevedelli, C., Regenfu, C., Riccardi, O., R?hne, A., Rotondi, H., Sandaker, Scampoli, Paola, J., Storey, M. A., Subieta Vasquez, M., ?pa?ek, G., Testera, E., Widmann, P., Yzombard, S., Zavatarelli, and J., Zmeskal
- Abstract
AE¯gIS experiment’s main goal is to measure the local gravitational acceleration of antihydrogen ¯g and thus perform a direct test of the weak equivalence principle with antimatter. In the first phase of the experiment the aim is to measure ¯g with 1% relative precision. This paper presents the antihydrogen production method and a description of some components of the experiment, which are necessary for the gravity measurement. Current status of the AE¯gIS experimental apparatus is presented and recent commissioning results with antiprotons are outlined. In conclusion we discuss the short-term goals of the AE¯gIS collaboration that will pave the way for the first gravity measurement in the near future.
- Published
- 2014
30. Effects of current density on the formation and microstructure of Sn–9Zn, Sn–8Zn–3Bi and Sn–3Ag–0.5Cu solder joints
- Author
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Ahmad Badri Ismail, B.D. Long, T. Ariga, D.N. Binh, and Radzali Othman
- Subjects
Materials science ,Mechanical Engineering ,Metallurgy ,Metals and Alloys ,Intermetallic ,General Chemistry ,Substrate (electronics) ,Microstructure ,Anode ,Mechanics of Materials ,Soldering ,Materials Chemistry ,Growth rate ,Current density ,Joint (geology) - Abstract
The formation and growth of intermetallic compounds (IMCs) between lead-free solder alloys and Cu substrate were investigated. Cu6Sn5 IMC was formed in the Sn–3Ag–0.5Cu solder joint, whilst Cu5Zn8 IMC was formed in the Sn–9Zn and Sn–8Zn–3Bi solder joints after soldering. After exposure to a current density of 500 A/cm2 and 100 °C for 120 h, a sub-layer was detected in the Sn–3Ag–0.5Cu solder joint and this was identified as IMC Cu3Sn. The growth of the IMCs increased with increasing current density and was found to be faster at the anode side. Under the same testing conditions, the results showed that the growth rate or the thickness of the IMCs was highest in Sn–9Zn, followed by Sn–8Zn–3Bi, and the least being in Sn–3Ag–0.5Cu. The microstructure of Sn–3Ag–0.5Cu solder joint was observed to exhibit changes under exposure to current, whilst the microstructure of the Sn–9Zn and Sn–8Zn–3Bi solder joints remain unchanged, except for the increase in IMCs thickness.
- Published
- 2012
- Full Text
- View/download PDF
31. New results on νμ → ντ appearance with the OPERA experiment in the CNGS beam
- Author
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. Badertscher, A. Ben Dhahbi, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, G. Brunetti, B. Büttner, S. Buontempo, L. Chaussard, M. Chernyavskiy, V. Chiarella, A. Chukanov, L. Consiglio, N. D’Ambrosio, P. Amo Sanchez, G. Lellis, M. Serio, A. Crescenzo, D. Ferdinando, N. Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, J. Ebert, A. Ereditato, J. Favier, T. Ferber, R. A. Fini, T. Fukuda, A. Garfagnini, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, A. M. Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, H. Kawahara, J. Kawada, J. H. Kim, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, A. Meregaglia, P. Migliozzi, S. Mikado, A. Minotti, M. Miyanishi, E. Miyashita, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, T. Roganova, H. Rokujo, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt Parzefall, I. Shakiryanova, T. Schcedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strauss, P. Strolin, K. Suzuki, S. Takahashi, F. Terranova, V. Tioukov, P. Tolun, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche, GIACOMELLI, GIORGIO MARIA, MAURI, NICOLETTA, MEDINACELI VILLEGAS, EDUARDO, SIOLI, MAXIMILIANO, TENTI, MATTEO, N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, T. Asada, D. Autiero, A. Badertscher, A. Ben Dhahbi, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, G. Brunetti, B. Büttner, S. Buontempo, L. Chaussard, M. Chernyavskiy, V. Chiarella, A. Chukanov, L. Consiglio, N. D’Ambrosio, P. Amo Sanchez, G. Lelli, M. Serio, A. Crescenzo, D. Ferdinando, N. Marco, S. Dmitrievski, M. Draco, D. Duchesneau, S. Dusini, J. Ebert, A. Ereditato, J. Favier, T. Ferber, R. A. Fini, T. Fukuda, A. Garfagnini, G. Giacomelli, C. Goellnitz, J. Goldberg, Y. Gornushkin, G. Grella, F. Grianti, A. M Guler, C. Gustavino, C. Hagner, K. Hakamata, T. Hara, T. Hayakawa, M. Hierholzer, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, M. Ishikawa, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, T. Katsuragawa, H. Kawahara, J. Kawada, J. H. Kim, S. H. Kim, M. Kimura, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, G. Mandrioli, J. Marteau, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, P. Migliozzi, S. Mikado, A. Minotti, M. Miyanishi, E. Miyashita, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, A. Pastore, L. Patrizii, E. Pennacchio, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, K. Pretzl, F. Pupilli, R. Rescigno, M. Roda, T. Roganova, H. Rokujo, G. Rosa, I. Rostovtseva, A. Rubbia, A. Russo, O. Ryazhskaya, O. Sato, Y. Sato, A. Schembri, W. Schmidt-Parzefall, I. Shakiryanova, T. Schcedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, T. Strau, P. Strolin, K. Suzuki, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, P. Tolun, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, J. Yoshida, M. Yoshimoto, Y. Zaitsev, S. Zemskova, A. Zghiche, DE LELLIS, Giovanni, Lauria, Adele, Montesi, MARIA CRISTINA, DI CRESCENZO, Antonia, DIP. DI FISICA, DIPARTIMENTO DI FISICA E ASTRONOMIA 'AUGUSTO RIGHI', Facolta' di SCIENZE MATEMATICHE FISICHE e NATURALI, Da definire, AREA MIN. 02 - Scienze fisiche, Agafonova, N, Aleksandrov, A, Anokhina, A, Aoki, S, Ariga, A, Ariga, T, Asada, T, Autiero, D, Badertscher, A, Dhahbi, A, Bender, D, Bertolin, A, Bozza, C, Brugnera, R, Brunetti, G, Büttner, B, Buontempo, S, Chaussard, L, Chernyavskiy, M, Chiarella, V, Chukanov, A, Consiglio, L, D’Ambrosio, N, Del Amo Sanchez, P, De Lellis, G, De Serio, M, Di Crescenzo, A, Di Ferdinando, D, Di Marco, N, Dmitrievski, S, Dracos, M, Duchesneau, D, Dusini, S, Ebert, J, Ereditato, A, Favier, J, Ferber, T, Fini, R, Fukuda, T, Garfagnini, A, Giacomelli, G, Goellnitz, C, Goldberg, J, Gornushkin, Y, Grella, G, Grianti, F, Guler, A, Gustavino, C, Hagner, C, Hakamata, K, Hara, T, Hayakawa, T, Hierholzer, M, Hollnagel, A, Hosseini, B, Ishida, H, Ishiguro, K, Ishikawa, M, Jakovcic, K, Jollet, C, Kamiscioglu, C, Kamiscioglu, M, Katsuragawa, T, Kawahara, H, Kawada, J, Kim, J, Kim, S, Kimura, M, Kitagawa, N, Klicek, B, Kodama, K, Komatsu, M, Kose, U, Kreslo, I, Lauria, A, Lenkeit, J, Ljubicic, A, Longhin, A, Loverre, P, Malgin, A, Mandrioli, G, Marteau, J, Matsuo, T, Matveev, V, Mauri, N, Medinaceli, E, Meregaglia, A, Migliozzi, P, Mikado, S, Minotti, A, Miyanishi, M, Miyashita, E, Monacelli, P, Montesi, M, Morishima, K, Muciaccia, M, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Nakatsuka, Y, Niwa, K, Ogawa, S, Okateva, N, Olshevsky, A, Omura, T, Ozaki, K, Paoloni, A, Park, B, Park, I, Pastore, A, Patrizii, L, Pennacchio, E, Pessard, H, Pistillo, C, Podgrudkov, D, Polukhina, N, Pozzato, M, Pretzl, K, Pupilli, F, Rescigno, R, Roda, M, Roganova, T, Rokujo, H, Rosa, G, Rostovtseva, I, Rubbia, A, Russo, A, Ryazhskaya, O, Sato, O, Sato, Y, Schembri, A, Schmidt Parzefall, W, Shakiryanova, I, Schcedrina, T, Sheshukov, A, Shibuya, H, Shiraishi, T, Shoziyoev, G, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Spinetti, M, Stanco, L, Starkov, N, Stellacci, S, Stipcevic, M, Strauss, T, Strolin, P, Suzuki, K, Takahashi, S, Tenti, M, Terranova, F, Tioukov, V, Tolun, P, Tufanli, S, Vilain, P, Vladimirov, M, Votano, L, Vuilleumier, J, Wilquet, G, Wonsak, B, Yoon, C, Yoshida, J, Yoshimoto, M, Zaitsev, Y, Zemskova, S, and Zghiche, A
- Subjects
Nuclear and High Energy Physics ,Particle physics ,Neutrino detectors and telescopes ,NEUTRINO OSCILLATIONS ,530 Physics ,Physics::Instrumentation and Detectors ,CERN Neutrinos to Gran Sasso ,01 natural sciences ,NO ,Nuclear physics ,neutrino ,0103 physical sciences ,Oscillation ,Nuclear emulsion ,Nuclear Experiment ,010306 general physics ,Neutrino oscillation ,Charged current ,TAU LEPTON ,Physics ,Neutrino Detectors and Telescopes ,010308 nuclear & particles physics ,NEUTRINO DETECTORS ,Physique atomique et nucléaire ,PARTICLE PHYSICS ,NUCLEAR EMULSION ,Physique des particules élémentaires ,oscillation ,neutrino detectors and telescopes ,High Energy Physics::Experiment ,Neutrino ,Energy (signal processing) ,Beam (structure) - Abstract
The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the ν μ → ν τ channel, via the detection of the τ-leptons created in charged current ν τ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17 GeV. The observation of the first ν τ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ν τ candidate has been observed. The significance of the two events in terms of a ν μ → ν τ oscillation signal is of 2.40σ., Journal of High Energy Physics, 2013 (11), ISSN:1126-6708, ISSN:1029-8479
- Published
- 2013
- Full Text
- View/download PDF
32. EUV radiation characteristics of a CO2 laser produced Xe plasma
- Author
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G. Soumagne, T. Ariga, Akira Endo, Y. Ueno, H. Hoshino, Hiroshi Komori, and Hakaru Mizoguchi
- Subjects
Materials science ,Physics and Astronomy (miscellaneous) ,business.industry ,Plasma parameters ,Amplifier ,Extreme ultraviolet lithography ,Energy conversion efficiency ,General Engineering ,General Physics and Astronomy ,Plasma ,Radiation ,Laser ,Pulsed laser deposition ,law.invention ,Optics ,Physics::Plasma Physics ,law ,business - Abstract
A CO2 laser-driven Xe liquid jet plasma has been studied with respect to its usability as a EUV lithography light source. A short-pulse TEA-CO2 master oscillator power amplifier system (MOPA) and a pre-pulse Nd:YAG laser were used for the plasma generation. The dependence of EUV plasma parameters, e.g., conversion efficiency, plasma image, in-band and out-of-band spectra, on the delay time between the pre-pulse and the main pulse laser was investigated. A maximum conversion efficiency of 0.6% was obtained at a delay time of about 200 ns. In addition, characteristics of fast ions were measured by the time-of-flight method. The peak energy of the fast ion energy distribution decreased significantly at delay times longer than 200 ns. This result is very promising with respect to a collector mirror lifetime extension by magnetic field mitigation.
- Published
- 2006
- Full Text
- View/download PDF
33. Resonant behaviour of base-isolated high-rise buildings under long-period ground motions
- Author
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Izuru Takewaki, Yoshihiro Kanno, and T. Ariga
- Subjects
Engineering ,business.industry ,Base (geometry) ,Resonance ,Building and Construction ,Structural engineering ,Surface wave ,Long period ,Range (aeronautics) ,Architecture ,Frequency characteristic ,business ,Seismology ,Intensity (heat transfer) ,Civil and Structural Engineering ,High rise - Abstract
SUMMARY The resonant behaviour of base-isolated high-rise buildings under long-period ground motions is investigated. The long-period ground motions are known to be induced by surface waves. While the acceleration amplitude of such long-period ground motion is small, the velocity amplitude is fairly large. It is expected that high-rise buildings and base-isolated buildings with long fundamental natural periods are greatly influenced by these long-period ground motions. Especially base-isolated high-rise buildings with friction-type bearings may have remarkable mechanical characteristics unfavourable for these long-period ground motions. The purpose of this paper is to reveal that the long-period ground motions recorded in Japan have the intensity to make base-isolated high-rise buildings in resonance with long-period components and that careful treatment is inevitable in the structural design of these base-isolated high-rise buildings. It is pointed out that the friction-type bearings are effective in general in avoiding the resonance with ground motions with a narrow-range frequency characteristic, but are dangerous for ground motions with a wide-range frequency characteristic in the long period range. Copyright © 2005 John Wiley & Sons, Ltd.
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- 2006
- Full Text
- View/download PDF
34. Search for nu(mu) -> nu(tau) oscillation with the OPERA experiment in the CNGS beam
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N. AGAFONOVA, A. ALEKSANDROV, O. ALTINOK, A. ANOKHINA, S. AOKI, A. ARIGA, T. ARIGA, D. AUTIERO, A. BADERTSCHER, A. BAGULYA, A. BEN DHAHBI, A. BERTOLIN, C. BOZZA, T. BRUGIERE, R. BRUGNERA, F. BRUNET, G. BRUNETTI, S. BUONTEMPO, A. CAZES, L. CHAUSSARD, M. CHERNYAVSKIY, V. CHIARELLA, A. CHUKANOV, N. D’AMBROSIO, F. DAL CORSO, Y. DECLAIS, P. DEL AMO SANCHEZ, G. DE LELLIS, M. DE SERIO, F. DI CAPUA, A. DI CRESCENZO, D. DI FERDINANDO, N. DI MARCO, S. DMITRIEVSKI, M. DRACOS, D. DUCHESNEAU, S. DUSINI, T. DZHATDOEV, J. EBERT, O. EGOROV, R. ENIKEEV, A. EREDITATO, L. S. ESPOSITO, J. FAVIER, T. FERBER, R. A. FINI, D. FREKERS, T. FUKUDA, A. GARFAGNINI, C. GOLLNITZ, J. GOLDBERG, D. GOLUBKOV, L. GONCHAROVA, Y. GORNUSHKIN, G. GRELLA, F. GRIANTI, A. M. GULER, C. GUSTAVINO, C. HAGNER, K. HAMADA, T. HARA, M. HIERHOLZER, A. HOLLNAGEL, K. HOSHINO, M. IEVA, H. ISHIDA, K. ISHIGURO, K. JAKOVCIC, C. JOLLET, F. JUGET, M. KAMISCIOGLU, S. H. KIM, M. KIMURA, N. KITAGAWA, B. KLICEK, J. KNUESEL, K. KODAMA, K. KOGISO, M. KOMATSU, U. KOSE, I. KRESLO, C. LAZZARO, J. LENKEIT, I. LIPPI, A. LJUBICIC, A. LONGHIN, P. LOVERRE, G. LUTTER, A. MALGIN, G. MANDRIOLI, K. MANNAI, J. MARTEAU, T. MATSUO, V. MATVEEV, MAURI, NICOLETTA, E. MEDINACELI, F. MEISEL, A. MEREGAGLIA, P. MIGLIOZZI, S. MIKADO, S. MIYAMOTO, P. MONACELLI, K. MORISHIMA, U. MOSER, M. T. MUCIACCIA, N. NAGANAWA, T. NAKA, M. NAKAMURA, T. NAKANO, Y. NAKATSUKA, D. NAUMOV, V. NIKITINA, K. NIWA, Y. NONOYAMA, S. OGAWA, N. OKATEVA, A. OLSHEVSKY, T. OMURA, O. PALAMARA, M. PANICCIA, A. PAOLONI, B. D. PARK, I. G. PARK, A. PASTORE, L. PATRIZII, E. PENNACCHIO, H. PESSARD, C. PISTILLO, N. POLUKHINA, K. PRETZL, F. PUPILLI, R. RESCIGNO, T. ROGANOVA, H. ROKUJO, G. ROMANO, G. ROSA, I. ROSTOVTSEVA, A. RUBBIA, A. RUSSO, V. RYASNY, O. RYAZHSKAYA, O. SATO, Y. SATO, A. SCHEMBRI, W. SCHMIDT PARZEFALL, L. SCOTTO LAVINA, A. SHESHUKOV, H. SHIBUYA, G. SHOZIYOEV, S. SIMONE, C. SIRIGNANO, G. SIRRI, J. S. SONG, M. SPINETTI, L. STANCO, N. STARKOV, M. STELLACCI, M. STIPCEVIC, T. STRAUSS, P. STROLIN, K. SUZUKI, S. TAKAHASHI, M. TENTI, F. TERRANOVA, I. TEZUKA, V. TIOUKOV, P. TOLUN, A. TRABELSI, T. TRAN, S. TUFANLI, P. VILAIN, M. VLADIMIROV, L. VOTANO, J. L. VUILLEUMIER, G. WILQUET, B. WONSAK, V. YAKUSHEV, C. S. YOON, J. YOSHIDA, T. YOSHIOKA, Y. ZAITSEV, S. ZEMSKOVA, A. ZGHICHE, R. ZIMMERMANN, GIACOMELLI, GIORGIO MARIA, GIORGINI, MIRIAM, POZZATO, MICHELE, SIOLI, MAXIMILIANO, Agafonova, N, Aleksandrov, A, Altinok, O, Anokhina, A, Aoki, S, Ariga, A, Ariga, T, Autiero, D, Badertscher, A, Bagulya, A, Ben Dhahbi, A, Bertolin, A, Bozza, C, Brugière, T, Brugnera, R, Brunet, F, Brunetti, G, Buontempo, S, Cazes, A, Chaussard, L, Chernyavskiy, M, Chiarella, V, Chukanov, A, D'Ambrosio, N, Dal Corso, F, Déclais, Y, del Amo Sanchez, P, De Lellis, G, De Serio, M, Di Capua, F, Di Crescenzo, A, Di Ferdinando, D, Di Marco, N, Dmitrievski, S, Dracos, M, Duchesneau, D, Dusini, S, Dzhatdoev, T, Ebert, J, Egorov, O, Enikeev, R, Ereditato, A, Esposito, L, Favier, J, Ferber, T, Fini, R, Frekers, D, Fukuda, T, Garfagnini, A, Giacomelli, G, Giorgini, M, Göllnitz, C, Goldberg, J, Golubkov, D, Goncharova, L, Gornushkin, Y, Grella, G, Grianti, F, Guler, A, Gustavino, C, Hagner, C, Hamada, K, Hara, T, Hierholzer, M, Hollnagel, A, Hoshino, K, Ieva, M, Ishida, H, Ishiguro, K, Jakovcic, K, Jollet, C, Juget, F, Kamiscioglu, M, Kim, S, Kimura, M, Kitagawa, N, Klicek, B, Knuesel, J, Kodama, K, Kogiso, K, Komatsu, M, Kose, U, Kreslo, I, Lazzaro, C, Lenkeit, J, Lippi, I, Ljubicic, A, Longhin, A, Loverre, P, Lutter, G, Malgin, A, Mandrioli, G, Mannai, K, Marteau, J, Matsuo, T, Matveev, V, Mauri, N, Medinaceli, E, Meisel, F, Meregaglia, A, Migliozzi, P, Mikado, S, Miyamoto, S, Monacelli, P, Morishima, K, Moser, U, Muciaccia, M, Naganawa, N, Naka, T, Nakamura, M, Nakano, T, Nakatsuka, Y, Naumov, D, Nikitina, V, Niwa, K, Nonoyama, Y, Ogawa, S, Okateva, N, Olshevsky, A, Omura, T, Palamara, O, Paniccia, M, Paoloni, A, Park, B, Park, I, Pastore, A, Patrizii, L, Pennacchio, E, Pessard, H, Pistillo, C, Polukhina, N, Pozzato, M, Pretzl, K, Pupilli, F, Rescigno, R, Roganova, T, Rokujo, H, Romano, G, Rosa, G, Rostovtseva, I, Rubbia, A, Russo, A, Ryasny, V, Ryazhskaya, O, Sato, O, Sato, Y, Schembri, A, Schmidt Parzefall, W, Scotto Lavina, L, Sheshukov, A, Shibuya, H, Shoziyoev, G, Simone, S, Sioli, M, Sirignano, C, Sirri, G, Song, J, Spinetti, M, Stanco, L, Starkov, N, Stellacci, M, Stipcevic, M, Strauss, T, Strolin, P, Suzuki, K, Takahashi, S, Tenti, M, Terranova, F, Tezuka, I, Tioukov, V, Tolun, P, Trabelsi, A, Tran, T, Tufanli, S, Vilain, P, Vladimirov, M, Votano, L, Vuilleumier, J, Wilquet, G, Wonsak, B, Yakushev, V, Yoon, C, Yoshida, J, Yoshioka, T, Zaitsev, Y, Zemskova, S, Zghiche, A, Zimmermann, R, N. AGAFONOVA, A. ALEKSANDROV, O. ALTINOK, A. ANOKHINA, S. AOKI, A. ARIGA, T. ARIGA, D. AUTIERO, A. BADERTSCHER, A. BAGULYA, A. BEN DHAHBI, A. BERTOLIN, C. BOZZA, T. BRUGIERE, R. BRUGNERA, F. BRUNET, G. BRUNETTI, S. BUONTEMPO, A. CAZES, L. CHAUSSARD, M. CHERNYAVSKIY, V. CHIARELLA, A. CHUKANOV, N. D’AMBROSIO, F. DAL CORSO, Y. DECLAIS, P. DEL AMO SANCHEZ, G. DE LELLIS, M. DE SERIO, F. DI CAPUA, A. DI CRESCENZO, D. DI FERDINANDO, N. DI MARCO, S. DMITRIEVSKI, M. DRACOS, D. DUCHESNEAU, S. DUSINI, T. DZHATDOEV, J. EBERT, O. EGOROV, R. ENIKEEV, A. EREDITATO, L. S. ESPOSITO, J. FAVIER, T. FERBER, R. A FINI, D. FREKERS, T. FUKUDA, A. GARFAGNINI, G. GIACOMELLI, M. GIORGINI, C. GOLLNITZ, J. GOLDBERG, D. GOLUBKOV, L. GONCHAROVA, Y. GORNUSHKIN, G. GRELLA, F. GRIANTI, A. M. GULER, C. GUSTAVINO, C. HAGNER, K. HAMADA, T. HARA, M. HIERHOLZER, A. HOLLNAGEL, K. HOSHINO, M. IEVA, H. ISHIDA, K. ISHIGURO, K. JAKOVCIC, C. JOLLET, F. JUGET, M. KAMISCIOGLU, S. H. KIM, M. KIMURA, N. KITAGAWA, B. KLICEK, J. KNUESEL, K. KODAMA, K. KOGISO, M. KOMATSU, U. KOSE, I. KRESLO, C. LAZZARO, J. LENKEIT, I. LIPPI, A. LJUBICIC, A. LONGHIN, P. LOVERRE, G. LUTTER, A. MALGIN, G. MANDRIOLI, K. MANNAI, J. MARTEAU, T. MATSUO, V. MATVEEV, N. MAURI, E. MEDINACELI, F. MEISEL, A. MEREGAGLIA, P. MIGLIOZZI, S. MIKADO, S. MIYAMOTO, P. MONACELLI, K. MORISHIMA, U. MOSER, M. T. MUCIACCIA, N. NAGANAWA, T. NAKA, M. NAKAMURA, T. NAKANO, Y. NAKATSUKA, D. NAUMOV, V. NIKITINA, K. NIWA, Y. NONOYAMA, S. OGAWA, N. OKATEVA, A. OLSHEVSKY, T. OMURA, O. PALAMARA, M. PANICCIA, A. PAOLONI, B. D. PARK, I. G. PARK, A. PASTORE, L. PATRIZII, E. PENNACCHIO, H. PESSARD, C. PISTILLO, N. POLUKHINA, M. POZZATO, K. PRETZL, F. PUPILLI, R. RESCIGNO, T. ROGANOVA, H. ROKUJO, G. ROMANO, G. ROSA, I. ROSTOVTSEVA, A. RUBBIA, A. RUSSO, V. RYASNY, O. RYAZHSKAYA, O. SATO, Y. SATO, A. SCHEMBRI, W. SCHMIDT-PARZEFALL, L. SCOTTO LAVINA, A. SHESHUKOV, H. SHIBUYA, G. SHOZIYOEV, S. SIMONE, M. SIOLI, C. SIRIGNANO, G. SIRRI, J. S. SONG, M. SPINETTI, L. STANCO, N. STARKOV, M. STELLACCI, M. STIPCEVIC, T. STRAUSS, P. STROLIN, K. SUZUKI, S. TAKAHASHI, M. TENTI, F. TERRANOVA, I. TEZUKA, V. TIOUKOV, P. TOLUN, A. TRABELSI, T. TRAN, S. TUFANLI, P. VILAIN, M. VLADIMIROV, L. VOTANO, J. L. VUILLEUMIER, G. WILQUET, B. WONSAK, V. YAKUSHEV, C. S. YOON, J. YOSHIDA, T. YOSHIOKA, Y. ZAITSEV, S. ZEMSKOVA, A. ZGHICHE, and R. ZIMMERMANN
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FIS/01 - FISICA SPERIMENTALE ,neutrino physics ,NEUTRINO ,FLAVOR OSCILLATIONS ,NUCLEAR EMULSIONS ,TAU LEPTON - Abstract
The OPERA neutrino experiment in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in direct appearance mode in the vμ→ v τ channel, the v τ signature being the identification of the τ -lepton created in its charged current interaction. The hybrid apparatus consists of a large mass emulsion film/lead target complemented by electronic detectors. Placed in the LNGS, it is exposed to the high-energy long-baseline CERN Neutrino beam to Gran Sasso (CNGS) 730 km away from the neutrino source. The observation of a first v τ candidate event was reported in 2010. In this paper, we discuss the result of the analysis of the data taken during the first two years of operation (2008-2009) underlining the major improvements brought to the analysis chain and to the Monte Carlo simulations. The statistical significance of the one event observed so far is then evaluated to 95%. © IOP Publishing Ltd and Deutsche Physikalische Gesellschaft.
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- 2012
35. An Ultra-Line-Narrowed High-Power<tex>$hboxF_2$</tex>Laser for Dioptric Design Microlithography Exposure Tools
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T. Ariga and H. Mizoguchi
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Range (particle radiation) ,Materials science ,business.industry ,Amplifier ,Laser ,Atomic and Molecular Physics, and Optics ,law.invention ,Power (physics) ,Full width at half maximum ,Laser linewidth ,Optics ,law ,Laser power scaling ,Electrical and Electronic Engineering ,business ,Energy (signal processing) - Abstract
An ultra-line-narrowed high-power and high-repetition rate F/sub 2/ laser system has been developed for 157-nm microlithography exposure tools with dioptric projection design. The injection locked system (ILS) consists of a low-power seed laser with ultra-narrow spectral linewidth and a high-gain amplifier. More than 25-W output power, a spectral linewidth below 0.2 pm full-width at half-maximum (FWHM) and an energy stability (3-sigma) below 10% have been obtained at a 5-kHz repetition rate and for a delay time range between the two laser stages of about 15 ns. Directly compared with a master oscillator power amplifier system, the ILS had a better performance related to output energy, energy stability, and laser pulse duration.
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- 2004
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36. R&D on nuclear emulsion detectors for muon radiography of large scale objects
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A. Ariga, T. Ariga, S. Braccini, A. Ereditato, F. Giacoppo, J. Kawada, I. Kreslo, C. Pistillo, SCAMPOLI, PAOLA, A., Ariga, T., Ariga, S., Braccini, A., Ereditato, F., Giacoppo, J., Kawada, I., Kreslo, C., Pistillo, and Scampoli, Paola
- Published
- 2011
37. Spectral dynamics of narrow-band F2 laser for optical lithography
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T. Ariga, Hiroki Tanaka, K. Hotta, R. Nohdomi, Tatsuo Okada, H. Mizoguchi, and Akihiko Takahashi
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Quantum optics ,Materials science ,Physics and Astronomy (miscellaneous) ,Computer simulation ,business.industry ,General Engineering ,Time evolution ,General Physics and Astronomy ,Laser ,law.invention ,Narrow band ,Optics ,law ,Code (cryptography) ,Emission spectrum ,Photolithography ,business - Abstract
We describe the spectral dynamics of a line-narrowed F2 laser, based on numerical simulation by a newly developed simulation code. The results were compared with the experimental results and it was found that the code could predict well the performance of a line-narrowed operation of the F2 laser. The code was also used to obtain a guideline for the optimized operation of an injection-seeded F2 laser system. In addition, a new spectral narrowing technique for the F2 laser has been proposed and its effectiveness was evaluated by the simulation code.
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- 2003
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38. Observation of a first ντ candidate event in the OPERA experiment in the CNGS beam
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N. AGAFONOVA, A. ALEKSANDROV, O. ALTINOK, M. AMBROSIO, A. ANOKHINA, S. AOKI, A. ARIGA, T. ARIGA, D. AUTIERO, A. BADERTSCHER, A. BAGULYA, A. BENDHABI, A. BERTOLIN, M. BESNIER, D. BICK, V. BOYARKIN, C. BOZZA, T. BRUGIERE, R. BRUGNERA, F. BRUNET, G. BRUNETTI, S. BUONTEMPO, A. CAZES, L. CHAUSSARD, M. CHERNYAVSKY, V. CHIARELLA, N. CHON SEN, A. CHUKANOV, R. CIESIELSKI, F. DAL CORSO, N. D’AMBROSIO, Y. DECLAIS, P. DEL AMO SANCHEZ, G. DE LELLIS, M. DE SERIO, F. DI CAPUA, A. DI CRESCENZO, D. DI FERDINANDO, N. DI MARCO, A. DI GIOVANNI, S. DMITRIEVSKY, M. DRACOS, D. DUCHESNEAU, S. DUSINI, T. DZHATDOEV, J. EBERT, O. EGOROV, R. ENIKEEV, A. EREDITATO, L. S. ESPOSITO, J. FAVIER, T. FERBER, R. A. FINI, D. FREKERS, T. FUKUDA, V. GALKIN, A. GARFAGNINI, J. GOLDBERG, C. GOLLNITZ, D. GOLUBKOV, L. GONCHAROVA, Y. GORNUSHKIN, G. GRELLA, F. GRIANTI, A. M. GULER, C. GUSTAVINO, C. HAGNER, K. HAMADA, T. HARA, M. HIERHOLZER, K. HOSHINO, M. IEVA, H. ISHIDA, K. ISHIGURO, K. JAKOVCIC, C. JOLLET, F. JUGET, M. KAMISCIOGLU, J. KAWADA, M. KAZUYAMA, S. H. KIM, M. KIMURA, N. KITAGAWA, B. KLICEK, J. KNUESEL, K. KODAMA, M. KOMATSU, U. KOSE, I. KRESLO, H. KUBOTA, C. LAZZARO, J. LENKEIT, I. LIPPI, A. LJUBICIC, A. LONGHIN, G. LUTTER, A. MALGIN, G. MANDRIOLI, K. MANNAI, A. MAROTTA, J. MARTEAU, T. MATSUO, V. MATVEEV, MAURI, NICOLETTA, E. MEDINACELI, F. MEISEL, A. MEREGAGLIA, P. MIGLIOZZI, S. MIKADO, S. MIYAMOTO, P. MONACELLI, K. MORISHIMA, U. MOSER, M. T. MUCIACCIA, N. NAGANAWA, T. NAKA, M. NAKAMURA, T. NAKANO, Y. NAKATSUKA, D. NAUMOV, V. NIKITINA, K. NIWA, Y. NONOYAMA, S. OGAWA, A. OLCHEVSKY, T. OMURA, G. ORLOVA, V. OSEDLO, M. PANICCIA, A. PAOLONI, B. D. PARK, I. G. PARK, A. PASTORE, L. PATRIZII, E. PENNACCHIO, H. PESSARD, V. PILIPENKO, C. PISTILLO, N. POLUKHINA, K. PRETZL, P. PUBLICHENKO, F. PUPILLI, J. P. REPELLIN, R. RESCIGNO, T. ROGANOVA, H. ROKUJO, G. ROMANO, G. ROSA, I. ROSTOVTSEVA, A. RUBBIA, A. RUSSO, V. RYASNY, O. RYAZHSKAYA, Y. SAKATANI, O. SATO, Y. SATO, A. SCHEMBRI, W. SCHMIDT PARZEFALL, H. SCHROEDER, L. SCOTTO LAVINA, A. SHESHUKOV, H. SHIBUYA, S. SIMONE, C. SIRIGNANO, G. SIRRI, J. S. SONG, M. SPINETTI, L. STANCO, N. STARKOV, M. STIPCEVIC, T. STRAUSS, P. STROLIN, K. SUZUKI, S. TAKAHASHI, M. TENTI, F. TERRANOVA, I. TEZUKA, V. TIOUKOV, P. TOLUN, A. TRABELSI, T. TRAN, S. TUFANLI, P. VILAIN, M. VLADIMIROV, L. VOTANO, J. L. VUILLEUMIER, G. WILQUET, B. WONSAK, V. YAKUSHEV, C. S. YOON, J. YOSHIDA, T. YOSHIOKA, Y. ZAITSEV, S. ZEMSKOVA, A. ZGHICHE, R. ZIMMERMANN, GIACOMELLI, GIORGIO MARIA, GIORGINI, MIRIAM, POZZATO, MICHELE, SIOLI, MAXIMILIANO, N. AGAFONOVA, A. ALEKSANDROV, O. ALTINOK, M. AMBROSIO, A. ANOKHINA, S. AOKI, A. ARIGA, T. ARIGA, D. AUTIERO, A. BADERTSCHER, A. BAGULYA, A. BENDHABI, A. BERTOLIN, M. BESNIER, D. BICK, V. BOYARKIN, C. BOZZA, T. BRUGIERE, R. BRUGNERA, F. BRUNET, G. BRUNETTI, S. BUONTEMPO, A. CAZES, L. CHAUSSARD, M. CHERNYAVSKY, V. CHIARELLA, N. CHON-SEN, A. CHUKANOV, R. CIESIELSKI, F.DAL CORSO, N. D’AMBROSIO, Y. DECLAIS, P. DEL AMO SANCHEZ, G. DE LELLIS, M. DE SERIO, F. DI CAPUA, A. DI CRESCENZO, D. DI FERDINANDO, N. DI MARCO, A. DI GIOVANNI, S. DMITRIEVSKY, M. DRACOS, D. DUCHESNEAU, S. DUSINI, T. DZHATDOEV, J. EBERT, O. EGOROV, R. ENIKEEV, A. EREDITATO, L.S. ESPOSITO, J. FAVIER, T. FERBER, R.A. FINI, D. FREKERS, T. FUKUDA, V. GALKIN, A. GARFAGNINI, G. GIACOMELLI, M. GIORGINI, J. GOLDBERG, C. GOLLNITZ, D. GOLUBKOV, L. GONCHAROVA, Y. GORNUSHKIN, G. GRELLA, F. GRIANTI, A.M. GULER, C. GUSTAVINO, C. HAGNER, K. HAMADA, T. HARA, M. HIERHOLZER, K. HOSHINO, M. IEVA, H. ISHIDA, K. ISHIGURO, K. JAKOVCIC, C. JOLLET, F. JUGET, M. KAMISCIOGLU, J. KAWADA, M. KAZUYAMA, S.H. KIM, M. KIMURA, N. KITAGAWA, B. KLICEK, J. KNUESEL, K. KODAMA, M. KOMATSU, U. KOSE, I. KRESLO, H. KUBOTA, C. LAZZARO, J. LENKEIT, I. LIPPI, A. LJUBICIC, A. LONGHIN, G. LUTTER, A. MALGIN, G. MANDRIOLI, K. MANNAI, A. MAROTTA, J. MARTEAU, T. MATSUO, V. MATVEEV, N. MAURI, E. MEDINACELI, F. MEISEL, A. MEREGAGLIA, P. MIGLIOZZI, S. MIKADO, S. MIYAMOTO, P. MONACELLI, K. MORISHIMA, U. MOSER, M.T. MUCIACCIA, N. NAGANAWA, T. NAKA, M. NAKAMURA, T. NAKANO, Y. NAKATSUKA, D. NAUMOV, V. NIKITINA, K. NIWA, Y. NONOYAMA, S. OGAWA, A. OLCHEVSKY, T. OMURA, G. ORLOVA, V. OSEDLO, M. PANICCIA, A. PAOLONI, B.D. PARK, I.G. PARK, A. PASTORE, L. PATRIZII, E. PENNACCHIO, H. PESSARD, V. PILIPENKO, C. PISTILLO, N. POLUKHINA, M. POZZATO, K. PRETZL, P. PUBLICHENKO, F. PUPILLI, J.P. REPELLIN, R. RESCIGNO, T. ROGANOVA, H. ROKUJO, G. ROMANO, G. ROSA, I. ROSTOVTSEVA, A. RUBBIA, A. RUSSO, V. RYASNY, O. RYAZHSKAYA, Y. SAKATANI, O. SATO, Y. SATO, A. SCHEMBRI, W. SCHMIDT-PARZEFALL, H. SCHROEDER, L. SCOTTO LAVINA, A. SHESHUKOV, H. SHIBUYA, S. SIMONE, M. SIOLI, C. SIRIGNANO, G. SIRRI, J.S. SONG, M. SPINETTI, L. STANCO, N. STARKOV, M. STIPCEVIC, T. STRAUSS, P. STROLIN, K. SUZUKI, S. TAKAHASHI, M. TENTI, F. TERRANOVA, I. TEZUKA, V. TIOUKOV, P. TOLUN, A. TRABELSI, T. TRAN, S. TUFANLI, P. VILAIN, M. VLADIMIROV, L. VOTANO, J.-L. VUILLEUMIER, G. WILQUET, B. WONSAK, V. YAKUSHEV, C.S. YOON, J. YOSHIDA, T. YOSHIOKA, Y. ZAITSEV, S. ZEMSKOVA, A. ZGHICHE, and R. ZIMMERMANN
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NEUTRINO OSCILLATIONS ,Physics::Instrumentation and Detectors ,PARTICLE PHYSICS ,High Energy Physics::Experiment ,Nuclear Experiment ,NUCLEAR EMULSIONS - Abstract
First observation of neutrino oscillation in appearance mode
- Published
- 2010
39. Autosomal-dominant Hypoplastic Form of Amelogenesis Imperfecta Caused by an Enamelin Gene Mutation at the Exon-Intron Boundary
- Author
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Tetsuo Shirakawa, T. Ariga, Haruhisa Oguchi, Miyuki Kida, and Y. Sakiyama
- Subjects
0301 basic medicine ,Proband ,Male ,Candidate gene ,Amelogenesis Imperfecta ,DNA Mutational Analysis ,Molecular Sequence Data ,Locus (genetics) ,Gene mutation ,Biology ,03 medical and health sciences ,Exon ,0302 clinical medicine ,Dental Enamel Proteins ,medicine ,Humans ,Amelogenesis imperfecta ,Child ,General Dentistry ,Polymorphism, Single-Stranded Conformational ,Genes, Dominant ,Genetics ,Base Sequence ,Guanosine ,FAM83H ,030206 dentistry ,Exons ,medicine.disease ,Molecular biology ,Introns ,Pedigree ,030104 developmental biology ,Codon, Nonsense ,Female ,ENAM ,Chromosomes, Human, Pair 4 - Abstract
Amelogenesis imperfecta (AI) is currently classified into 14 distinct subtypes based on various phenotypic criteria; however, the gene responsible for each phenotype has not been defined. We performed molecular genetic studies on a Japanese family with a possible autosomal-dominant form of AI. Previous studies have mapped an autosomal-dominant human AI locus to chromosome 4q11-q21, where two candidate genes, ameloblastin and enamelin, are located. We studied AI patients in this family, focusing on these genes, and found a mutation in the enamelin gene. The mutation detected was a heterozygous, single-G deletion within a series of 7 G residues at the exon 9-intron 9 boundary of the enamelin gene. The mutation was detected only in AI patients in the family and was not detected in other unaffected family members or control individuals. The male proband and his brother showed hypoplastic enamel in both their deciduous and permanent teeth, and their father showed local hypoplastic defects in the enamel of his permanent teeth. The clinical phenotype of these patients is similar to that of the first report of AI caused by an enamelin gene mutation. Thus, heterogeneous mutations in the enamelin gene are responsible for an autosomal-dominant hypoplastic form of AI.
- Published
- 2002
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40. Effect of Copper-based Fillers Composition On Spreading and Wetting Behaviour
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Tedi Kurniawan, Mahadzir Ishak, W. N. W. M. N. Hissyam, A. M. Halil, and T Ariga
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010302 applied physics ,Materials science ,Alloy ,chemistry.chemical_element ,02 engineering and technology ,engineering.material ,021001 nanoscience & nanotechnology ,01 natural sciences ,Copper ,Contact angle ,Sessile drop technique ,chemistry ,Filler (materials) ,0103 physical sciences ,engineering ,Brazing ,Wetting ,Composite material ,0210 nano-technology ,Base metal - Abstract
Wetting and spreading of molten brazing filler material are important factors that influence the brazing ability of a joint to be brazed. Several investigations into the wetting ability of a brazing filler alloy and its spreading area in the molten state, in addition to effects of brazing temperature on the contact angle, have been carried out. Generally, the composition of copper-based filler and temperature affect spreading of molten brazing filler material during brazing. Wetting by and interfacial reactions of the molten brazing filler material with the metallic substrate, especially, affect strongly the spreading of the filler material. In this study, the effects of filler composition and brazing temperature on the spreading of molten brazing filler metallic alloys were investigated. MBF 2005 (Cu, 5.7wt.%Ni, 9.7wt.%Sn, 7.0wt.%P), MBF 2002 (Cu, 9.9wt.%Ni, 4.0wt.%Sn, 7.8wt.%P) and VZ 2250 (Cu, 7.0wt.%Ni, 9.3wt.%Sn, 6.3wt.%P) alloys were used as brazing filler materials. Pure copper block and a rectangular plate were employed as the base metal. Brazing filler material and metallic base plate were first washed with acetone. Brazing was performed at 750°C and 800°C under Ar gas for 30 minutes using an electrically heated furnace, after which, the original spreading area, defined as the sessile drop area, and the apparent spreading area were both evaluated. It was observed that the spreading area and wetting angle influenced by the composition of copper-based filler.
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- 2017
- Full Text
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41. Measurement of the TeV atmospheric muon charge ratio with the complete OPERA data set
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N. Agafonova, A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, D. Bender, A. Bertolin, C. Bozza, R. Brugnera, A. Buonaura, S. Buontempo, B. Büttner, M. Chernyavsky, A. Chukanov, L. Consiglio, N. D’Ambrosio, G. De Lellis, M. De Serio, P. Del Amo Sanchez, A. Di Crescenzo, D. Di Ferdinando, N. Di Marco, S. Dmitrievski, M. Dracos, D. Duchesneau, S. Dusini, T. Dzhatdoev, J. Ebert, A. Ereditato, R. A. Fini, T. Fukuda, G. Galati, A. Garfagnini, G. Giacomelli, C. Göllnitz, J. Goldberg, Y. Gornushkin, G. Grella, M. Guler, C. Gustavino, C. Hagner, T. Hara, A. Hollnagel, B. Hosseini, H. Ishida, K. Ishiguro, K. Jakovcic, C. Jollet, C. Kamiscioglu, M. Kamiscioglu, J. Kawada, J. H. Kim, S. H. Kim, N. Kitagawa, B. Klicek, K. Kodama, M. Komatsu, U. Kose, I. Kreslo, A. Lauria, J. Lenkeit, A. Ljubicic, A. Longhin, P. Loverre, A. Malgin, M. Malenica, G. Mandrioli, T. Matsuo, V. Matveev, N. Mauri, E. Medinaceli, A. Meregaglia, S. Mikado, P. Monacelli, M. C. Montesi, K. Morishima, M. T. Muciaccia, N. Naganawa, T. Naka, M. Nakamura, T. Nakano, Y. Nakatsuka, K. Niwa, S. Ogawa, N. Okateva, A. Olshevsky, T. Omura, K. Ozaki, A. Paoloni, B. D. Park, I. G. Park, L. Pasqualini, A. Pastore, L. Patrizii, H. Pessard, C. Pistillo, D. Podgrudkov, N. Polukhina, M. Pozzato, F. Pupilli, M. Roda, H. Rokujo, T. Roganova, G. Rosa, O. Ryazhskaya, O. Sato, A. Schembri, I. Shakiryanova, T. Shchedrina, A. Sheshukov, H. Shibuya, T. Shiraishi, G. Shoziyoev, S. Simone, M. Sioli, C. Sirignano, G. Sirri, M. Spinetti, L. Stanco, N. Starkov, S. M. Stellacci, M. Stipcevic, P. Strolin, S. Takahashi, M. Tenti, F. Terranova, V. Tioukov, S. Tufanli, P. Vilain, M. Vladimirov, L. Votano, J. L. Vuilleumier, G. Wilquet, B. Wonsak, C. S. Yoon, S. Zemskova, and A. Zghiche
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Physics ,Particle physics ,Muon ,Physics and Astronomy (miscellaneous) ,Physics::Instrumentation and Detectors ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Detector ,Cosmic ray ,01 natural sciences ,symbols.namesake ,Pion ,Magnet ,0103 physical sciences ,symbols ,Feynman diagram ,High Energy Physics::Experiment ,010306 general physics ,Nucleon ,Engineering (miscellaneous) ,Scaling - Abstract
The OPERA detector, designed to search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scale cosmic rays. For the analysis here presented, the detector was used to measure the atmospheric muon charge ratio in the TeV region. OPERA collected charge-separated cosmic ray data between 2008 and 2012. More than 3 million atmospheric muon events were detected and reconstructed, among which about 110000 multiple muon bundles. The charge ratio $R_{\mu} \equiv N_{\mu^+}/N_{\mu^-}$ was measured separately for single and for multiple muon events. The analysis exploited the inversion of the magnet polarity which was performed on purpose during the 2012 Run. The combination of the two data sets with opposite magnet polarities allowed minimizing systematic uncertainties and reaching an accurate determination of the muon charge ratio. Data were fitted to obtain relevant parameters on the composition of primary cosmic rays and the associated kaon production in the forward fragmentation region. In the surface energy range 1-20 TeV investigated by OPERA, $R_{\mu}$ is well described by a parametric model including only pion and kaon contributions to the muon flux, showing no significant contribution of the prompt component. The energy independence supports the validity of Feynman scaling in the fragmentation region up to $200$ TeV/nucleon primary energy.
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- 2014
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42. The AEgIS Experiment
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A. Knecht, S. Aghion, O. Ahlxe9n, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, G. Bonomi, P. Brxe4unig, J. Bremer, R. S. Brusa, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, J. H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Haider, S. D. Hogan, T. Huse, E. Jordan, L. V. Jxf8rgensen, T. Kaltenbacher, and J. Kawada
- Published
- 2014
43. Measuring the gravitational free-fall of antihydrogen
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J. Storey, S. Aghion, O. Ahlxe9n, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, G. Bonomi, P. Brxe4unig, J. Bremer, R. S. Brusa, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, J. H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Haider, S. D. Hogan, T. Huse, E. Jordan, L. V. Jxf8rgensen, T. Kaltenbacher, and J. Kawada
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- 2014
44. Measuring with , progress and perspectives
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D. Krasnickxfd, S. Aghion, O. Ahlxe9n, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, K. Berggren, G. Bonomi, P. Brxe4unig, J. Bremer, R. S. Brusa, L. Cabaret, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Haider, T. Huse, E. Jordan, L. V. Jxf8rgensen, T. Kaltenbacher, and J. Kawada
- Published
- 2014
45. AE$\overline {\rm{g}}$IS Experiment: Measuring the accelerationgof the earth’s gravitational field on antihydrogen beam
- Author
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M. A. Subieta Vasquez, S. Aghion, O. Ahlén, C. Amsler, A. Ariga, T. Ariga, A. S. Belov, G. Bonomi, P. Bräunig, J. Bremer, R. S. Brusa, L. Cabaret, M. Caccia, C. Canali, R. Caravita, F. Castelli, G. Cerchiari, S. Cialdi, D. Comparat, G. Consolati, L. Dassa, J. H. Derking, S. Di Domizio, L. Di Noto, M. Doser, A. Dudarev, A. Ereditato, R. Ferragut, A. Fontana, P. Genova, M. Giammarchi, A. Gligorova, S. N. Gninenko, S. Heider, S. D. Hogan, T. Huse, E. Jordan, L. V. Jørgensen, T. Kaltenbacher, J. Kawada, A. Kellerbauer, M. Kimura, A. Knecht, D. Krasnický, V. Lagomarsino, S. Mariazzi, V. A. Matveev, F. Merkt, F. Moia, G. Nebbia, P. Nédélec, M. K. Oberthaler, N. Pacifico, V. Petráček, C. Pistilo, F. Prelz, M. Prevedelli, C. Regenfus, C. Ricardi, O. Røhne, A. Rotondi, H. Sandaker, P. Scampoli, J. Storey, M. Špaček, G. Testera, D. Trezzi, R. Vaccarone, F. Villa, and S. Zavatarelli
- Subjects
Physics ,Particle physics ,QC1-999 ,Electron ,Gravitational acceleration ,7. Clean energy ,Nuclear physics ,Antiproton Decelerator ,Deflection (physics) ,Antiproton ,Antimatter ,Physics::Accelerator Physics ,Physics::Atomic Physics ,Antihydrogen ,Beam (structure) - Abstract
The AEg¯ $\overline {\rm{g}}$IS experiment [1] aims at directly measuring the gravitational acceleration g on a beam of cold antihydrogen (H¯$\overline {\rm{H}}$) to a precision of 1%, performing the first test with antimatter of the (WEP) Weak Equivalence Principle. The experimental apparatus is sited at the Antiproton Decelerator (AD) at CERN, Geneva, Switzerland. After production by mixing of antiprotons with Rydberg state positronium atoms (Ps), the H¯$\overline {\rm{H}}$ atoms will be driven to fly horizontally with a velocity of a few 100 ms−1 for a path length of about 1 meter. The small deflection, few tens of μm, will be measured using two material gratings (of period ∼ 80 μm) coupled to a position-sensitive detector working as a moiré deflectometer similarly to what has been done with matter atoms [2]. The shadow pattern produced by the H¯$\overline {\rm{H}}$ beam will then be detected by reconstructing the annihilation points with a spatial resolution (∼ 2 μm) of each antiatom at the end of the flight path by the sensitive-position detector. During 2012 the experimental apparatus has been commissioned with antiprotons and positrons. Since the AD will not be running during 2013,during the refurbishment of the CERN accelerators, the experiment is currently working with positrons, electrons and protons, in order to prepare the way for the antihydrogen production in late 2014.
- Published
- 2014
46. Protective effects of murine recombinant interferon-β administered by intravenous, intramuscular or subcutaneous route on mouse hepatitis virus infection
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T. Ariga, T. Kikuchi, F. Taguchi, S. Matsuyama, S. Sone, S. Henmi, and N. Ichihara
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Male ,Coronaviridae Infections ,Injections, Subcutaneous ,Injections, Intramuscular ,Virus ,Mice ,Route of administration ,Mouse hepatitis virus ,Nidovirales ,Virology ,Animals ,Medicine ,Interferon gamma ,Pharmacology ,Hepatitis ,Mice, Inbred BALB C ,biology ,business.industry ,biology.organism_classification ,medicine.disease ,Recombinant Proteins ,Liver ,Hepatitis, Viral, Animal ,Injections, Intravenous ,Interferon Type I ,Immunology ,Viral disease ,business ,Viral hepatitis ,medicine.drug - Abstract
The significance of the route for administration of murine recombinant interferon-beta (IFN-beta) for inducing its therapeutic effects has been studied. BALB/c mice were daily injected intravenously, intramuscularly or subcutaneously with 1.5x10(3), 1. 5x10(4), or 1.5x10(5) IU of IFN-beta, from one day before to 8th day after mouse hepatitis virus (MHV-2) challenge. All mice received IFN-beta survived significantly longer than those without IFN. In the liver of those IFN-treated mice, viral growth and the histopathological damages were extremely alleviated. These results suggest that, irrespective of the differences in the route of administration, IFN-beta markedly suppressed viral activity when its administration was started prior to viral infection. For clinical use, however, further studies are needed on the optimal route for administration if IFN-beta is given after viral infection.
- Published
- 2000
- Full Text
- View/download PDF
47. Characterization of glycosphingolipids by direct inlet chemical ionization mass spectrometry
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T Ariga, T Murata, M Oshima, M Maezawa, and T Miyatake
- Subjects
Biochemistry ,QD415-436 - Abstract
Permethylated derivatives of cerebrosides and ceramide di-, tri-, tetra-, and penta-hexosides were analyzed by the direct inlet ammonia chemical ionization (CI) mass spectrometry. In the CI mass spectra, the fragment ions produced by the loss of methanol from the protonated molecular ion were observed in all of the glycosphingolipids. Other fragment ions due to the cleavage of glycosidic moiety were major ones under the CI conditions. These ions provide information on the molecular species of glycosphingolipids and the sugar sequence of their oligosaccharides. Glycosphingolipids with hydroxy fatty acids could also be differentiated from those with nonhydroxy fatty acids by comparing the intensities of characteristic fragment ions. The CI method should be particularly useful in structural studies of glycosphingolipids from natural sources.
- Published
- 1980
- Full Text
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48. Characterization of GM1 ganglioside by direct inlet chemical ionization mass spectrometry.
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T Ariga, R K Yu, M Suzuki, S Ando, and T Miyatake
- Subjects
Biochemistry ,QD415-436 - Abstract
Intact permethylated and permethylated-reduced (LiAlH4) derivatives of GM1 ganglioside were analyzed by direct inlet ammonia chemical ionization (CI) mass spectrometry. In addition, the trimethylsilylated derivative of the permethylated-reduced sample of this ganglioside was similarly analyzed. CI mass spectrometry proves to be a highly satisfactory method for structural studies of GM1 ganglioside because of the simple fragmentation pattern and the presence of prominent molecular ions and fragment ions in the high mass region. Complete information on the carbohydrate sequence and lipophilic composition can be easily obtained.
- Published
- 1982
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49. Characterization of trimethylsilyl derivatives of cerebrosides by direct inlet-chemical ionization mass spectrometry.
- Author
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T Murata, T Ariga, M Oshima, and T Miyatake
- Subjects
Biochemistry ,QD415-436 - Abstract
Submicrogram quantities of trimethylsilyl derivatives of cerebrosides obtained from the spleen of a patient with Gaucher's disease and from bovine brain were analyzed by direct probe inlet-chemical ionization mass spectrometry, using isobutane as the reagent gas. Quasimolecular ions (QM+, M + 73) and other recognizable fragment ions produced by the successive elimination of trimethylsilanol and sugar residue gave useful information about fatty acid compositions. These ions could also be utilized for qualitative analyses of the molecular species of cerebrosides. Cerebrosides with non-hydroxy and hydroxy fatty acids could be discriminated from each other by comparing the intensities of their quasimolecular ions. Cerebrosides with saturated and monounsaturated fatty acids could also be discrimnated from each other, because the mass number decreased by two mass units in cerebrosides with monounsaturated fatty acids. It was concluded that structural information and molecular species determination could be obtained from small amounts of purified cerebrosides.
- Published
- 1978
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50. Determination of double bond positions of unsaturated fatty acids by a chemical ionization mass spectrometry computer system
- Author
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T Murata, T Ariga, and E Araki
- Subjects
trimethylsilylated methyl ester ,stereospecific oxidation ,Biochemistry ,QD415-436 - Abstract
After stereospecific oxidation, trimethylsilylated methyl esters of mono- and diunsaturated fatty acids were analyzed by combined gas–liquid chromatography–chemical ionization mass spectrometry. The positions of original double bonds were deduced from the fragment ions produced by the cleavage of the carbon–carbon bond between two trimethylsilyl ethers. These fragment ions were recorded at m/e 187 and 259 in the case of 16:1(n-7), at m/e 187 and 287 in the case of 18:1(n-7), at m/e 215 and 259 in the case of 18:1(n-9), and at m/e 172 and 259 in the case of 18:2(n-6), respectively. The diastereoisomers of monounsaturated fatty acids can be discriminated by comparing the intensities of the fragment ions at m/e 253 and 285 in the case of 16:1 and at m/e 281 and 313 in the case of 18:1. The diastereosiomers of diunsaturated fatty acids may also be distinguished from each other by comparing the intensities of the fragment ions formed by the loss of trimethylsilyl function from the characteristic ions. Mono- and diunsaturated fatty acids in liver may be dominantly in cis- 18:1(n-1) and cis-cis-18:2(n-6) as determined by a mass chromatographic technique.
- Published
- 1978
- Full Text
- View/download PDF
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