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Showing papers by "G. Tzanakos published in 2002"


Journal ArticleDOI
TL;DR: In this article, a new method of emulsion analysis, NETSCAN, was used to locate neutrino events and detect tau decays, which achieved plate-to-plate alignment accuracy of ∼0.2 μm over an area of 2.6 mm × 2.2 mm.
Abstract: The DONUT experiment used an emulsion/counter-hybrid-detector, which succeeded in detecting tau–neutrino charged-current interactions. A new method of emulsion analysis, NETSCAN, was used to locate neutrino events and detect tau decays. It is based on a fully automated emulsion readout system (Ultra Track Selector) developed at Nagoya University. The achieved plate-to-plate alignment accuracy of ∼0.2 μm over an area of 2.6 mm ×2.6 mm permitted an efficient and systematic tau decay search using emulsion data. Moreover, this accuracy allowed measurement of particle momenta by multiple Coulomb scattering, and contributed to the efficient background rejection for the ντ candidates. This paper describes details of our emulsion analysis methods.

85 citations


ReportDOI
D. S. Ayres, Alexandre Lebedev, Karol Lang, E. Blucher, D. G. Michael, N.V. Mokhov, H. S. Budd, J. L. Thron, G. F. Pearce, A. C. Weber, T. Patzak, D. E. Reyna, G.D. Barr, A. De Santo, S. Pordes, Gary Drake, I. Trostin, A. Marchionni, D. A. Harris, D.S. Carman, S. Menary, C. Cueva, E. Kearns, W. Metcalf, Kirk T. McDonald, P. Shanahan, V. Makeev, Marvin L Marshak, A. Bodek, G. Ginther, C.R. Brune, S. Manly, J. Schneps, R. L. Talaga, G. J. Feldman, K.H. Hicks, K. S. McFarland, P. J. Litchfield, K. M. Heeger, K. Lee, C. Bromberg, Walter Winter, R. Svoboda, N. Morgan, V. Paolone, Juergen Thomas, J. Hylen, Raymond Lee, Kate Scholberg, Caren Hagner, David Petyt, G. M. Irwin, W. Sakumoto, P. M. Border, Stephen J. Parke, Kai Zuber, Adam Para, S. M. Seun, G. Tzanakos, B. Kayser, J. K. Nelson, T. Joffe-Minor, Patrick Huber, R. Hatcher, V. Scarpino, N. Giokaris, V. J. Guarino, D. M. DeMuth, K-B. Luk, A.K. Opper, P. Slattery, P. Lucas, J. Cooper, Philip Harris, Sacha E Kopp, N. Tagg, T. Kafka, J. Urheim, Alec Habig, H. J. Kang, R. A. Richards, Carl H. Albright, E. A. Peterson, S. Childress, B. C. Choudhary, D. Carey, H. Minakata, R. Imlay, C. W. Walter, Thomas R. Chase, M. Zielinski, P. Kasper, F. DeJongh, S.M. Grimes, David B. Cline, Ken Heller, Manfred Lindner, N. Pearson, Stanley G. Wojcicki, P. deBarbaro, L. Mualem, K. Ruddick, R. Ray, R. Shrock, A. Mann, J.H. Cobb, Panagiotis Spentzouris, D. Naples, S. M. S. Kasahara, H. R. Gallagher, S. Geer, M. C. Goodman, S. Avvakumov, Hiroshi Nunokawa, V. Ryabov 
TL;DR: The first phase of the proposed program includes a new detector, optimized for neutrino detection, with a fiducial mass of the order of 20 kton and exposed to neutrinos and antineutrino beams.
Abstract: The NuMI neutrino beam line and the MINOS experiment represent a major investment of US High Energy Physics in the area of neutrino physics. The forthcoming results could decisively establish neutrino oscillations as the underlying physics mechanism for the atmospheric $ umu$ deficit and provide a precise measurement of the corresponding oscillation parameters, $\dmsq23$ and $\sinsq2t23$.neutrino sector may well be within our reach. The full potential of the NuMI neutrino beam can be exploited by complementing the MINOS detector, under construction, with a new detector(s) placed at some off-axis position and collecting data in parallel with MINOS. The first phase of the proposed program includes a new detector, optimized for $ ue$ detection, with a fiducial mass of the order of 20 kton and exposed to neutrino and antineutrino beams. In a five year run its sensitivity to the $ umutonue$ oscillations will be at least a factor of ten beyond the current limit. The future direction of the program will depend on the results of this first phase, but it is very likely that it will be a combination of a significant increase of the neutrino beam intensity via an upgraded proton source and an increase of the detector mass by a factor of five or so. Depending on the circumstances, the goals of Phase II may be a further increase of the sensitivity of a search for $ umutonue$ oscillations, or, perhaps, a measurement of the CP violating phase $\delta$ in the lepton sector.

54 citations


Journal ArticleDOI
TL;DR: The development of the mammographic x-ray source model is presented, accompanied by a set of simulation studies concerning the influence of magnification effects as well as that of the x-rays spatial and spectral distribution on the mammography spatial resolution for a certain magnification factor (m = 1.4).
Abstract: A simulation model of mammographic x-ray sources with finite size has been developed. The model is based on Monte Carlo methods and it takes into account the electron penetration inside the anode, the anode geometry and material, as well as the resulting heel effect and the spectral and spatial distribution of x-rays. This x-ray source simulation model has been embedded into an earlier developed simulation package of a mammography unit. The main outputs of this model are Monte Carlo generated images that correspond to the irradiation of properly designed phantoms. In this way it is possible to make studies of the influence of x-ray source characteristics on MTF. This paper presents the development of the mammographic x-ray source model, accompanied by a set of simulation studies concerning the influence of magnification effects as well as that of the x-ray spatial and spectral distribution on the mammographic spatial resolution for a certain magnification factor (m = 1.4). The validity level of the model, as well as its limitations and perspectives, rise through comparisons with experimental and theoretical data.

26 citations