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20681por Önengüt, G, Van Dantzig, R, De Jong, M, Oldeman, R G C, Güler, M, Köse, U, Tolun, P, Catanesi, M G, Muciaccia, M T, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Goldberg, J, Hristova, I R, Kawamura, T, Kolev, D, Kayis-Topaksu, A, Meinhard, H, Panman, J, Rozanov, A, Tsenov, R V, Zucchelli, P, Uiterwijk, J W E, Chikawa, M, Song, J S, Yoon, C S, Kodama, K, Ushida, N, Hara, T, Aoki, S, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Makhlyoueva, I V, Bruski, N, Frekers, D, Tsukerman, I, Shamanov, V V, Khovanskii, V D, Gorbunov, P, Artamonov, A V, Sato, Y, Tezuka, I, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Dore, U, Loverre, P F, Ludovici, L, Rosa, G, Santacesaria, R, Satta, A, Spada, F R, Okusawa, T, Hoshino, K, Kawada, J, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A G, D'Ambrosio, N, De Lellis, G, De Rosa, G, Di Capua, F, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Scotto-Lavina, L, Strolin, P, Tioukov, V“…During the years 1994-97, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy. In total about 100 000 charged-current neutrino interactions were located in the nuclear emulsion target and fully reconstructed. …”
Publicado 2005
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20682por Kayis-Topaksu, A, Önengüt, G, Van Dantzig, R, De Jong, M, Oldeman, R G C, Güler, M, Köse, U, Tolun, P, Catanesi, M G, Muciaccia, M T, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Hristova, I R, Kawamura, T, Kolev, D, Meinhard, H, Panman, J, Rozanov, A, Tsenov, R V, Uiterwijk, J W E, Zucchelli, P, Goldberg, J, Chikawa, M, Song, J S, Yoon, C S, Kodama, K, Ushida, N, Aoki, S, Hara, T, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Makhlyoueva, I V, Artamonov, A V, Gorbunov, P, Khovanskii, V D, Shamanov, V V, Tsukerman, I, Bruski, N, Frekers, D, Hoshino, K, Kawada, J, Komatsu, M, Myanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A G, D'Ambrosio, N, De Lellis, G, De Rosa, G, Di Capua, F, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Scotto-Lavina, L, Strolin, P, Tioukov, V, Okusawa, T, Dore, U, Loverre, P F, Ludovici, L, Rosa, G, Santacesaria, R, Satta, A, Spada, F R, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, Tezuka, I“…Selecting only events with visible energy greater than 30 GeV gives a value of Bμ that is less affected by the charm production threshold and quasi-elastic _+ c production. …”
Publicado 2005
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20683por Mitrovski, Michael K., Alt, C., Anticic, T., Baatar, B., Barna, D., Bartke, J., Betev, L., Bialkowska, H., Blume, C., Boimska, B., Botje, M., Bracinik, J., Bramm, R., Buncic, P., Cerny, V., Christakoglou, P., Chung, P., Chvala, O., Cramer, J.G., Csato, P., Dinkelaker, P., Eckardt, V., Flierl, D., Fodor, Z., Foka, P., Friese, V., Gal, J., Gazdzicki, M., Genchev, V., Georgopoulos, G., Gladysz, E., Grebieszkow, K., Hegyi, S., Hohne, C., Kadija, K., Karev, A., Kikola, D., Kliemant, M., Kniege, S., Kolesnikov, V.I., Kornas, E., Korus, R., Kowalski, M., Kraus, I., Kreps, M., Laszlo, A., Lacey, R., van Leeuwen, M., Levai, P., Litov, L., Lungwitz, B., Makariev, M., Malakhov, A.I., Mateev, M., Melkumov, G.L., Meurer, C., Mischke, A., Molnar, J., Mrowczynski, St., Nicolic, V., Palla, G., Panagiotou, A.D., Panayotov, D., Petridis, A., Peryt, W., Pikna, M., Pluta, J., Prindle, D., Puhlhofer, F., Renfordt, R., Roland, C., Roland, G., Rybczynski, M., Rybicki, A., Sandoval, A., Schmitz, N., Schuster, T., Seyboth, P., Sikler, F., Sitar, B., Skrzypczak, E., Slodkowski, M., Stefanek, G., Stock, R., Strabel, C., Strobele, H., Susa, T., Szentpetery, I., Sziklai, J., Szuba, M., Szymanski, P., Trubnikov, V., Varga, D., Vassiliou, M., Veres, G.I., Vesztergombi, G., Vranic, D., Wetzler, A., Wlodarczyk, Z., Yoo, I.K., Zimanyi, J.“…We present a summary of measurements of strange particles performed by the experiment NA49 in central and minimum bias Pb+Pb collisions in the beam energy range 20A - 158A GeV. New results on $\Xi$ production in central Pb+Pb collisions and on $\Lambda, \Xi$ production in minimum bias collisions are shown. …”
Publicado 2006
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20684por Kaneda, Michiru“…The mini black hole signals for n = 2 to 7 and M D = 0 . 8 GeV to 2 TeV are searched for. For each n and M D , the mass thresholds of the mini black holes were set by the assumptions that colliding particles collapse in a black hole if the Compton wavelength is equal to or less than the Schwarzschild radius or horizon radius. …”
Publicado 2015
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20685por Bogomilov, M, Matev, R, Tsenov, R, Dracos, M, Bonesini, M, Palladino, V, Tortora, L, Mori, Y, Planche, T, Lagrange, J B, Kuno, Y, Benedetto, E, Efthymiopoulos, I, Garoby, R, Gilardoini, S, Martini, M, Wildner, E, Prior, G, Blondel, A, Karadzhow, Y, Ellis, M, Kyberd, P, Bayes, R, Laing, A, Soler, F J P, Alekou, A, Apollonio, M, Aslaninejad, M, Bontoiu, C, Jenner, L J, Kurup, A, Long, K, Pasternak, J, Zarrebini, A, Poslimski, J, Blackmore, V, Cobb, J, Tunnell, C, Andreopoulos, C, Bennett, J R J, Brooks, S, Caretta, O, Davenne, T, Densham, C, Edgecock, T R, Fitton, M, Kelliher, D, Loveridge, P, McFarland, A, Machida, S, Prior, C, Rees, G, Rogers, C, Rooney, M, Thomason, J, Wilcox, D, Booth, C, Skoro, G, Back, J J, Harrison, P, Berg, J S, Fernow, R, Gallardo, J C, Gupta, R, Kirk, H, Simos, N, Stratakis, D, Souchlas, N, Witte, H, Bross, A, Geer, S, Johnstone, C, Mokhov, N, Neuffer, D, Popovic, M, Strait, J, Striganov, S, Morfín, J G, Wands, R, Snopok, P, Bogacz, S A, Morozov, V, Roblin, Y, Cline, D, Ding, X, Bromberg, C, Hart, T, Abrams, R J, Ankenbrandt, C M, Beard, K B, Cummings, M A C, Flanagan, G, Johnson, R P, Roberts, T J, Yoshikawa, C Y, Graves, V B, McDonald, K T, Coney, L, Hanson, G“…The EURO$\nu$ baseline accelerator facility will provide 10$^{21}$ muon decays per year from 12.6 GeV stored muon beams serving a single neutrino detector situated at a source-detector distance of between 1500 km and 2500 km. …”
Publicado 2014
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20686por Engl, Albert“…The single tube resolution of these 15 mm drift tubes was determined to be 95 m at the H8 test facility at CERN using a muon beam with an energy of 140 GeV.…”
Publicado 2016
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20687por Dräger, Arne-Rasmus“…The production of light-flavor $\tilde{\text{q}}$ below a mass of 780 GeV and $\tilde{\text{g}}$ with masses below 1.1-1.2 TeV are excluded at 95\% confidence level. …”
Publicado 2016
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20688por Marco-Hernández, Ricardo, Alves, D, Angoletta, M E, Marqversen, O, Molendijk, J, Oponowicz, E, Ruffieux, R, Sánchez-Quesada, J, Søby, L“…The AD machine at European Organization for Nuclear Research (CERN) is presently being used to decelerate antiprotons from 3.57 GeV/c to 100 MeV/c for matter vs anti-matter comparative studies. …”
Publicado 2017
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20689por Radhakrishnan, Sooraj“…The ridge correlations are found to persist to high pT (⇠10 GeV). Fourier harmonics up to order 5 are measured and found to be non-zero. …”
Publicado 2017
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20690por Lopez Paredes, Brais“…It is also applied in the search for Higgs decays to a Z boson and a photon, H → Zγ, introducing a 2% improvement in the upper limit set by the analysis, yielding 11 × S M at mH = 125.5 GeV (95% CL). The method is also used in the measurement of the photon electromagnetic scale to provide a precision better than 0.5%, reducing the measured Higgs mass systematic uncertainty obtained from the H → γγ analysis. …”
Publicado 2018
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20691por Kovalchuk, Nataliia“…The top quark mass is measured to be $m_{t} = 172.25 \pm0.08 \mbox{ (stat+JSF)}\pm0.62\mbox{ (syst) GeV}$. The results are tested for possible kinematic dependence by performing measurements of the top quark mass in different phase space regions.The residual data-to-simulation calibration of the energy of the jets is also estimated from dijet events with data collected at center-of-mass energy of 13 TeV in 2015 with the CMS detector corresponding to an integrated luminosity of 2.1 fb$^{-1}$. …”
Publicado 2018
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20692“…For this purpose, experiments were carried out at the CERN HiRadMat (High Radiation to Materials) facility in which extended solid copper cylindrical targets were irradiated with the 440 GeV proton beam generated by the Super Proton Synchrotron (SPS). …”
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20693por Nie, Y, Fichera, C, Mettler, L, Carra, F, Schmidt, R, Tahir, N A, Bertarelli, A, Wollmann, D“…This paper reports a benchmarking study against beam experiments performed at the HiRadMat (High-Radiation to Materials) facility using beams at 440 GeV from the Super Proton Synchrotron. Good agreement has been found between the simulation results and the experiments as well as previous simulations with fluka and big2 [Tahir et al., Phys. …”
Publicado 2019
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20694por Arnold, Oliver Werner“…These pairs were produced in reaction of p+Nb, where the proton had a kinetic energy of 3.5 GeV. At the beginning, all experimental correlation function were corrected for various detector effects. …”
Publicado 2019
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20695“…The SHiP experiment (for Search for Hidden Particles) which will operate at the CERN Super Proton Synchrotron (SPS) is one of the most promising projects in the field of particle physics. The SPS 400-GeV/c proton beam will be dumped onto the molybdenum–tungsten target of the SHiP detector, and the data corresponding to $2 \times 10^{20}$ protons on the target will be accumulated in five years of running. …”
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20696por Heister, Arno“…For quite low masses (50 < mH0 < 130[ GeV]) )1 the Higgs will predominantly decay into two b-quarks. …”
Publicado 2007
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20697por Missirian, Victor, Conklin, Phillip A., Culligan, Kevin M., Huefner, Neil D., Britt, Anne B.“…Here we study the effects of two different types of ionizing radiation (IR) treatment, HZE (1 GeV Fe(26+) high mass, high charge, and high energy relativistic particles) and gamma photons, on the transcriptome of Arabidopsis thaliana seedlings. …”
Publicado 2014
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20698por Adinolfi, M., Aglieri Rinella, G., Albrecht, E., Bellunato, T., Benson, S., Blake, T., Blanks, C., Brisbane, S., Brook, N. H., Calvi, M., Cameron, B., Cardinale, R., Carson, L., Contu, A., Coombes, M., D’Ambrosio, C., Easo, S., Egede, U., Eisenhardt, S., Fanchini, E., Fitzpatrick, C., Fontanelli, F., Forty, R., Frei, C., Gandini, P., Gao, R., Garra Tico, J., Giachero, A., Gibson, V., Gotti, C., Gregson, S., Gys, T., Haines, S. C., Hampson, T., Harnew, N., Hill, D., Hunt, P., John, M., Jones, C. R., Johnson, D., Kanaya, N., Katvars, S., Kerzel, U., Kim, Y. M., Koblitz, S., Kucharczyk, M., Lambert, D., Main, A., Maino, M., Malde, S., Mangiafave, N., Matteuzzi, C., Mini’, G., Mollen, A., Morant, J., Mountain, R., Morris, J. V., Muheim, F., Muresan, R., Nardulli, J., Owen, P., Papanestis, A., Patel, M., Patrick, G. N., Perego, D. L., Pessina, G., Petrolini, A., Piedigrossi, D., Plackett, R., Playfer, S., Powell, A., Rademacker, J. H., Ricciardi, S., Rogers, G. J., Sail, P., Sannino, M., Savidge, T., Sepp, I., Sigurdsson, S., Soler, F. J. P., Solomin, A., Soomro, F., Sparkes, A., Spradlin, P., Storaci, B., Thomas, C., Topp-Joergensen, S., Torr, N., Ullaland, O., Vervink, K., Voong, D., Websdale, D., Wilkinson, G., Wotton, S. A., Wyllie, K., Xing, F., Young, R.“…This provides charged particle identification over a wide momentum range, from 2–100 GeV/c. The operation and control, software, and online monitoring of the RICH system are described. …”
Publicado 2013
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20699“…At the NASA Space Radiation Laboratory (NSRL), we have proposed a GCR simulator, which implements a new rapid switching mode and higher energy beam extraction to 1.5 GeV/u, in order to integrate multiple ions into a single simulation within hours or longer for chronic exposures. …”
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20700por Li, X, Selesnick, RS, Baker, DN, Jaynes, AN, Kanekal, SG, Schiller, Q, Blum, L, Fennell, J, Blake, JB“…No instruments in the inner radiation belt are immune from the unforgiving penetration of the highly energetic protons (tens of MeV to GeV). The inner belt proton flux level, however, is relatively stable; thus, for any given instrument, the proton contamination often leads to a certain background noise. …”
Publicado 2015
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