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20802por Antel, C., Battaglieri, M., Beacham, J., Boehm, C., Buchmüller, O., Calore, F., Carenza, P., Chauhan, B., Cladè, P., Coloma, P., Crivelli, P., Dandoy, V., Darmé, L., Dey, B., Deppisch, F.F., De Roeck, A., Drewes, M., Echenard, B., Flambaum, V.V., Foldenauer, P., Gatti, C., Giannotti, M., Golutvin, A., Gonzalez-Garcia, M.C., Gori, S., Goudzovski, E., Granelli, A., Grote, H., Guellati-Khelifa, S., Hajer, J., Harris, P., Hearty, C., Heuchel, D., Hostert, M., Junius, S., Kahlhoefer, F., Klaric, J., Kling, F., Klose, P., Knolle, J., Kopp, J., Kwon, O., Lantwin, O., Lanfranchi, G., Li, L., Lindner, A., Lopez-Pavon, J., Marocco, J., Martin, J.W., Middleton, S., Milstead, S., Oceano, I., O'Hare, C.A.J., Paoloni, A., Pascoli, S., Petcov, S.T., Pospelov, M., Pöttgen, R., Raggi, M., Ripellino, G., Samsonov, I.B., Sandner, S., Söldner-Rembold, S., Shelton, J., Song, N., Sun, C., Stadnik, Y.V., Tastet, J.-L., Toro, N., Tran, N., Trevisani, N., Ulmer, S., Urrea, S., Velghe, B., Wallisch, B., Wong, Y.Y.Y., Zorbilmez, C., Zurek, K.“…Perhaps the most striking frontier to emerge in the search for answers involves new physics at mass scales comparable to familiar matter, below the GeV-scale, or even radically below, down to sub-eV scales, and with very feeble interaction strength. …”
Publicado 2023
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20803por Adeva, B, Akdogan, T, Arik, E, Arvidson, A, Badelek, B, Bardin, G, Baum, G, Berglund, P, Betev, L, Birsa, R, Björkholm, P, De Botton, N R, Boutemeur, M, Bradamante, Franco, Bravar, A, Bressan, A, Bültmann, S, Burtin, E, Cavata, C, Crabb, D, Cranshaw, J, Çuhadar-Dönszelmann, T, Dalla Torre, S, Van Dantzig, R, Derro, B R, Deshpande, A A, Dhawan, S K, Dulya, C M, Dyring, A, Eichblatt, S, Faivre, Jean-Claude, Fasching, D, Feinstein, F, Fernández, C, Forthmann, S, Frois, Bernard, Gallas, A, Garzón, J A, Gilly, H, Giorgi, M A, von Goeler, E, Görtz, S, Golutvin, I A, Gracia, G, De Groot, N, Grosse-Perdekamp, M, Haft, K, Von Harrach, D, Hasegawa, T, Hautle, P, Hayashi, N, Heusch, C A, Horikawa, N, Hughes, V W, Igo, G, Ishimoto, S, Iwata, T, Kabuss, E M, Kageya, T, Karev, A G, Kessler, H J, Ketel, T, Kiryluk, J, Kiryushin, Yu T, Kishi, A, Kiselev, Yu F, Klostermann, L, Krämer, Dietrich, Krivokhizhin, V G, Kröger, W, Kukhtin, V V, Kurek, K, Kyynäräinen, J, Lamanna, M, Landgraf, U, Le Goff, J M, Lehár, F, de Lesquen, A, Lichtenstadt, J, Lindqvist, T, Litmaath, M, Loewe, M, Magnon, A, Mallot, G K, Marie, F, Martin, A, Martino, J, Matsuda, T, Mayes, B W, McCarthy, J S, Medved, K S, Meyer, W T, Van Middelkoop, G, Miller, D, Miyachi, Y, Mori, K, Moromisato, J H, Nagaitsev, A P, Nassalski, J P, Naumann, Lutz, Niinikoski, T O, Oberski, J, Ogawa, A, Ozben, C, Pereira, H, Perrot-Kunne, F, Peshekhonov, V D, Piegia, R, Pinsky, L, Platchkov, S K, Pló, M, Pose, D, Postma, H, Pretz, J, Puntaferro, R, Pussieux, T, Rädel, G, Rijllart, A, Reicherz, G, Roberts, J, Rock, S E, Rodríguez, M, Rondio, Ewa, Ropelewski, Leszek, Sabo, I, Saborido, J, Sandacz, A, Savin, I A, Schiavon, R P, Schiller, A, Schüler, K P, Seitz, R, Semertzidis, Y K, Sergeev, S, Shanahan, P, Sichtermann, E P, Simeoni, F, Smirnov, G I, Staude, A, Steinmetz, A, Stiegler, U, Stuhrmann, H B, Szleper, M, Tessarotto, F, Thers, D, Tlaczala, W, Tripet, A, Ünel, G, Velasco, M, Vogt, J, Voss, Rüdiger, Whitten, C, Windmolders, R, Willumeit, R, Wislicki, W, Witzmann, A, Ylöstalo, J, Zanetti, A M, Zaremba, K, Zamiatin, N I, Zhao, J“…We present the final results of the spin asymmetries $A_1$ and the spin structure functions $g_1$ of the proton and the deuteron in the kinematic range $0.0008<x<0.7$ and $0.2<Q^2<100$ GeV$^2$. For the determination of $A_1$, in addition to the usual method which employs inclusive scattering events and includes a large radiative background at low $x$, we use a new method which minimizes t he radiative background by selecting events with at least one hadron as well as a muon in the final state. …”
Publicado 1998
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20804por Creanza, D, De Palma, M., Girone, M., Maggi, G., Selvaggi, G., Silvestris, L., Raso, G., Tempesta, P., Burns, M., Coyle, P., Engster, C., Frank, M., Moneta, L., Wachnik, M., Wagner, A., Zaslavsky, J., Focardi, E., Sguazzoni, G., Parrini, G., Scarlini, E., Halley, A., O'Shea, V., Raine, C., Barber, G., Cameron, W., Dornan, P., Gentry, D., Konstantinidis, N., Moutoussi, A., Nash, J., Price, D., Stacey, A., Toudup, L.W., Williams, M.I., Billault, M., Bonissent, A., Bujosa, G., Calvet, D., Carr, J., Diaconu, C., Blanc, P.E., Destelle, J.J., Karst, P., Payre, P., Rousseau, D., Thulasidas, M., Dietl, H., Moser, H.G., Settles, R., Seywerd, H., Waltermann, G., Bettarini, S., Bosi, F., Dell'Orso, R., Messineo, A., Profeti, A., Rizzo, G., Verdini, P.G., Walsh, J., Bizzell, J.P., Maley, P.D., Thompson, J.C., Wright, A.E., Black, S., Kim, H.Y., Bosisio, L., Putz, J., Rothberg, J., Wasserbaech, S., Elmer, P.“…An almost complete version of the upgraded VDET was installed in ALEPH during a three week LEP technical stop and took data in November 1995 during the LEP run at 130 GeV. The new detector worked well showing high signal over noise ratio and good efficiency. …”
Publicado 1997
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20805por Barton, R A, Afanasiev, S V, Anticic, T, Bächler, J, Barna, D, Barnby, L S, Bartke, Jerzy, Betev, L, Bialkowska, H, Billmeier, A, Blume, C, Blyth, C O, Boimska, B, Botje, M, Bracinik, J, Brady, F P, Bramm, R, Brun, R, Buncic, P, Carr, L, Cebra, D, Cooper, G E, Cramer, J G, Csató, P, Eckhardt, F, Ferenc, D, Filip, P, Fischer, H G, Fodor, Z, Foka, P Y, Freund, P, Friese, V, Ftácnik, J, Gál, J, Gazdzicki, M, Georgopoulos, G, Gladysz-Dziadus, E, Hegyi, S, Hlinka, V, Höhne, C, Igo, G, Ivanov, M, Jacobs, P, Janik, R, Jones, P G, Kadija, K, Kolesnikov, V I, Kollegger, T, Kowalski, M, Van Leeuwen, M, Lévai, Peter, Malakhov, A I, Margetis, S, Markert, C, Mayes, B W, Melkumov, G L, Mischke, A, Molnár, J, Nelson, J M, Odyniec, Grazyna Janina, Pálla, G, Panagiotou, A D, Petridis, A, Pikna, M, Pinsky, L, Poskanzer, A M, Prindle, D J, Pühlhofer, F, Reid, J G, Renfordt, R E, Retyk, W, Ritter, H G, Röhrich, D, Roland, C, Roland, G, Rybicki, A, Sammer, T, Sandoval, A, Sann, H, Schäfer, E, Schmitz, N, Seyboth, P, Siklér, F, Sitár, B, Skrzypczak, E, Snellings, R, Squier, G T A, Stock, Reinhard, Strmen, P, Ströbele, H, Susa, T, Szarka, I, Szentpétery, I, Sziklai, J, Toy, M, Trainor, T A, Trentalange, S, Varga, D, Vassiliou, Maria, Veres, G I, Vesztergombi, G, Voloshin, S A, Vranic, D, Wang, F, Weerasundara, D D, Wenig, S, Wetzler, A, Whitten, C, Xu, N, Yates, T A, Yoo, I K, Zimányi, J“…Preliminary results for the transverse mass and rapidity distributions for X and Xi /sup +/ from central Pb+Pb collisions at 158 GeV c/sup -1//nudeon are presented. Fully integrated yields per event of 4.42+or-0.31 and 0.74+0.04 are found for Xi /sup -/ and Xi /sup +/, respectively, leading to a 4 pi Xi /sup +// Xi /sup -/ ratio of 0.17+or-0.02. …”
Publicado 2001
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20806por Batley, J R, Kalmus, G E, Munday, D J, Wotton, S, Monnier, E, Winston, R, Gudzovskiy, E, Gurev, D, Hristov, P Z, Kuz'Min, N, Madigozhin, D, Pis'Mennyy, R, Potrebenikov, Y, Slepnev, I, Rubin, P D, Szleper, M, Dalpiaz, P, Damiani, C, Gianoli, A, Savrie, M, Wahl, H, Calvetti, M, Iacopini, E, Lenti, M, Veltri, M, Bocquet, G, Bremer, J, Cattai, A, Ceccucci, A, Formenti, F, Gatignon, L, Osmic, F, Panzer-Steindel, B, Piccini, M, Ruggiero, G, Unal, G P, Bloch-Devaux, B, De Beer, M, Debu, P, Derre, J, Gouge, G, Legou, P, Marel, G, Mazzucato, E, Peyaud, B, Vallage, B, Behler, M, Eppard, K, Kleinknecht, K, Masetti, L, Moosbrugger, U, Morales Morales, C, Renk, B, Wanke, R, Cornebise, P, Martin-Chassard, G, Anzivino, G, Cenci, P, Nappi, A, Papi, A, Pepe, M S, Petrucci, M C, Valdata, M, Cerri, C, Collazuol, G, Costantini, F, Fantechi, R, Ferrini, F, Mannelli, I, Raffaelli, G, Sozzi, M, Holder, M, Maier, A, Ziolkowski, M, Biino, C, Cartiglia, N, Cundy, D, Goy Lopez, S, Menichetti, E, Pastrone, N, Nassalski, J P, Dibon, H, Jeitler, M, Markytan, M, Neuhofer, G, Pernicka, M, Taurok, A“…This novel detector has fine transverse segmentation (2x2) cm$^{2}$, energy resolution better than 1% above 10~GeV shower energy and sub-nanosecond time resolution. …”
Publicado 2002
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20807por Astone, A“…This experiment is part of a global study over high power proton target, which includes also the experiment performed at BNL [9] in spri ng 2001 to achieve more detailed results and to use the different proton energy of 2.2 GeV. Experiments are requested in order to deliver bench marks for nu merical simulations [34]. …”
Publicado 2002
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20808por Alt, C., Anticic, T., Baatar, B., Barna, D., Bartke, J., Betev, L., Bialkowska, H., Billmeier, A., Blume, C., Boimska, B., Botje, M., Bracinik, J., Bramm, R., Brun, R., Buncic, P., Cerny, V., Christakoglou, P., Chvala, O., Cramer, J.G., Csato, P., Darmenov, N., Dimitrov, A., Dinkelaker, P., Eckardt, V., Farantatos, G., Flierl, D., Fodor, Z., Foka, P., Freund, P., Friese, V., Gal, J., Gazdzicki, M., Georgopoulos, G., Gladysz, E., Grebieszkow, K., Hegyi, S., Hohne, C., Kadija, K., Karev, A., Kliemant, M., Kniege, S., Kolesnikov, V.I., Kollegger, T., Kornas, E., Korus, R., Kowalski, M., Kraus, I., Kreps, M., van Leeuwen, M., Levai, P., Litov, L., Lungwitz, B., Makariev, M., Malakhov, A.I., Markert, C., Mateev, M., Mayes, B.W., Melkumov, G.L., Meurer, C., Mischke, A., Mitrovski, M., Molnar, J., Mrowczynski, St., Palla, G., Panagiotou, A.D., Panayotov, D., Petridis, A., Pikna, M., Pinsky, L., Puhlhofer, F., Reid, J.G., Renfordt, R., Richard, A., Roland, C., Roland, G., Rybczynski, M., Rybicki, A., Sandoval, A., Sann, H., Schmitz, N., Seyboth, P., Sikler, F., Sitar, B., Skrzypczak, E., Stefanek, G., Stock, R., Strobele, H., Susa, T., Szentpetery, I., Sziklai, J., Trainor, T.A., Varga, D., Vassiliou, M., Veres, G.I., Vesztergombi, G., Vranic, D., Wetzler, A., Wlodarczyk, Z., Yoo, I.K., Zaranek, J., Zimanyi, J.“…Results are presented on $\Omega$ production in central Pb+Pb collisions at 40 and 158A GeV beam energy. Given are transverse-mass spectra, rapidity distributions, and total yields for the sum $\Omega$+$\bar{\Omega}$ at 40 AGeV and for $\Omega$ and $\bar{\Omega}$ separately at 158 AGeV. …”
Publicado 2004
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20809por Kayis-Topaksu, A, Onengüt, G, Van Dantzig, R, De Jong, M, Melzer, O, Oldeman, R G C, Pesen, E, Spada, F R, Visschers, J L, Güler, M, Köse, U, Serin-Zeyrek, M, Sever, R, Tolun, P, Zeyrek, M T, Catanesi, M G, De Serio, M, Ieva, M, Muciaccia, M T, Radicioni, E, Simone, S, Bülte, A, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Pittoni, G L, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A V, Chizhov, M, Doucet, M, Hristova, I R, Kawamura, T, Kolev, D, Meinhard, H, Panman, J, Papadopoulos, I M, Ricciardi, S, Rozanov, A, Tsenov, R V, Uiterwijk, J W E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, 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, Gorbunov, P, Khovanskii, V D, Shamanov, V V, Tsukerman, I, Bruski, N, Frekers, D, 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, Ereditato, A, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Pistillo, C, Lavina, L S, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, Loverre, P F, Ludovici, L, Righini, P, Rosa, G, Santacesaria, R, Satta, A, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Sato, Y, Tezuka, I“…At the average neutrino energy of 27 GeV the cross-section for the total quasielastic production of charmed baryons relative to the nu N charged-current cross-section was measured to be sigma (QE)/ sigma (CC)=(0.23/sub -0.06//sup +0.12 /(stat)/sub -0.03//sup + /0/sup .02/(syst))*10/sup -2/. …”
Publicado 2003
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20810por Onengüt, G, Van Dantzig, R, De Jong, M, Konijn, J, Melzer, O, Oldeman, R G C, Pesen, E, Van der Poel, C A F J, Visschers, J L, Güler, M, Köse, U, Serin-Zeyrek, M, Kama, S, Sever, R, Tolun, P, Zeyrek, M T, Catanesi, M G, De Serio, M, Ieva, M, Muciaccia, M T, Radicioni, E, Simone, S, Bülte, A, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Artamonov, A V, Brunner, J, Chizhov, M, Cussans, D G, Doucet, M, Fabre, Jean-Paul, Hristova, I R, Kawamura, T, Kolev, D, Litmaath, M, Meinhard, H, Panman, J, Papadopoulos, I M, Ricciardi, S, Rozanov, A, Saltzberg, D, Tsenov, R V, Uiterwijk, J W E, Zucchelli, P, Goldberg, J, Chikawa, M, Arik, E, 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, Gorbunov, P, Khovanskii, V D, Shamanov, V V, Tsukerman, I, Bruski, N, Frekers, D, Rondeshagen, D, Wolff, 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, Ereditato, A, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Pistillo, C, Santorelli, R, Scotto-Lavina, L, Strolin, P, Tioukov, V, Nakamura, K, Okusawa, T, Dore, U, FLoverre, P, Ludovici, L, Maslennikov, A L, Righini, P, 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“…At an average antineutrino energy in the neutrino beam of 18GeV, the charm production rate induced by anitneutrinos is measured to be sigma(nubar_muN -> mu+cbarX)/sigma(nubar_muN -> mu+X) = (5.0^+1.4_-0.9(stat) +- 0.7(syst))%. …”
Publicado 2004
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20811por Emam, W S“…This dissertation reports on a precise measurement of the parity-violating asymmetry in electron-electron (Møller) scattering at a four-momentum transfer <italic>Q</italic><super>2</super> = 0.03 (GeV/c)<super>2</super>. The observed parity-violating asymmetry is <italic>A<sub>PV</sub></italic> = −128 ± 14 (stat.) …”
Publicado 2004
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20812por Mirra, Marco“…This work has been performed into the frame of the NA62 experiment at CERN that aims at measuring the Branching-Ratio of the ultra-rare kaon decay K+→π+ nu nubar with 10% uncertainty - using an unseparated kaon beam of 75GeV/c - in order to test the Standard Model (SM), to look for physics beyond SM and to measure the |Vtd| element of the Cabibbo-Kobayashi-Maskawa (CKM) flavor mixing matrix. …”
Publicado 2017
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20813por Chiaveri, E, Aberle, O, Andrzejewski, J, Audouin, L, Bacak, M, Balibrea, J, Barbagallo, M, Bečvář, F, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Caamaño, M, Calviño, F, Calviani, M, Cano-Ott, D, Cardella, R, Casanovas, A, Cerutti, F, Chen, Y H, Colonna, N, Cortés, G, Cortés-Giraldo, M A, Cosentino, L, Damone, L A, Diakaki, M, Domingo-Pardo, C, Dressler, R, Dupont, E, Durán, I, Fernández-Domínguez, B, Ferrari, A, Ferreira, P, Finocchiaro, P, Göbel, K, García, A R, Gawlik, A, Gilardoni, S, Glodariu, T, Gonçalves, I F, González, E, Griesmayer, E, Guerrero, C, Gunsing, F, Harada, H, Heinitz, S, Heyse, J, Jenkins, D G, Jericha, E, Käppeler, F, Kadi, Y, Kalamara, A, Kavrigin, P, Kimura, A, Kivel, N, Kokkoris, M, Krtička, M, Kurtulgil, D, Leal-Cidoncha, E, Lederer, C, Leeb, H, Lerendegui-Marco, J, Lo Meo, S, Lonsdale, S J, Macina, D, Marganiec, J, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Mastromarco, M, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Milazzo, P M, Mingrone, F, Musumarra, A, Negret, A, Nolte, R, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Porras, I, Praena, J, Quesada, J M, Radeck, D, Rauscher, T, Reifarth, R, Rubbia, C, Ryan, J A, Sabaté-Gilarte, M, Saxena, A, Schillebeeckx, P, Schumann, D, Smith, A G, Sosnin, N V, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A, Tassan-Got, L, Tsinganis, A, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vlachoudis, V, Vlastou, R, Wallner, A, Warren, S, Woods, P J, Wright, T, Žugec, P“…The CERN n_TOF neutron beam facility is characterized by a very high instantaneous neutron flux, excellent TOF resolution at the 185 m long flight path (EAR-1), low intrinsic background and coverage of a wide range of neutron energies, from thermal to a few GeV. These characteristics provide a unique possibility to perform high-accuracy measurements of neutron-induced reaction cross-sections and angular distributions of interest for fundamental and applied Nuclear Physics. …”
Publicado 2017
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20814por Moreels, Lieselotte“…The probability for this process to happen is reflected in the top quark decay width, which is predicted to have a value around 1.33 GeV. If the top quark is able to decay into other particles as well, as is possible in several extensions of the SM, the top quark decay width will be larger than the SM prediction. …”
Publicado 2018
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20815por Ruz, J, Vogel, J K, Armengaud, E, Attie, D, Basso, S, Brun, P, Bykovskiy, N, Carmona, J M, Castel, J F, Cebrián, S, Civitani, M, Cogollos, C, Costa, D, Dafni, T, Derbin, A V, Descalle, M A, Desch, K, Döbrich, B, Dratchnev, I, Dudarev, A, Ferrer-Ribas, E, Galán, J, Galanti, G, Gascón, D, Gastaldo, L, Garrido, L, Germani, C, Ghisellini, G, Giannotti, M, Giomataris, I, Gninenko, S, Golubev, N, Graciani, R, Irastorza, I G, Jakovčić, K, Kaminski, J, Krčmar, M, Krieger, C, Lakić, B, Lasserre, T, Laurent, P, Lomskaya, I, Unzhakov, E, Limousin, O, Lindner, A, Luzón, G, Mescia, F, Miralda-Escudé, J, Mirallas, H, Muratova, V N, Navick, X F, Nones, C, Notari, A, Nozik, A, Núñez, A, de Solórzano, A Ortiz, Pantuev, V, Papaevangelou, T, Pareschi, G, Picatoste, E, Pivovaroff, M J, Perez, K, Redondo, J, Ringwald, A, Ruiz-Chóliz, E, Salvadó, J, Schiffer, T, Schmidt, S, Schneekloth, U, Schott, M, Silva, H, Tagliaferri, G, Tavecchio, F, Ten Kate, H, Tkackev, I, Troitsky, S, Vedrine, P, Weltman, A“…BabyIAXO is proposed as an intermediate-scale experiment increasing the sensitivity to axion-photon couplings down to a few 10$^{−11}$ GeV$^{−1}$ and thus delivering significant physics results while demonstrating the feasibility of the full-scale IAXO experiment. …”
Publicado 2019
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20816por Sahr, Oliver“…In dieser Arbeit werden Messungen der Multiplizitat¨ und des Impulsspektrums geladener Teilchen, der Multiplizitat¨ schwerer Hadronen und die Messung des Teilchenflusses in W-Paar Ereignissen, die mit dem OPAL-Experiment bei Schwerpunktsenergien von 189 GeV aufgenommen wurden, beschrieben. Die gemessenen Werte in reinhadronischen Ereignissen werden mit Vorhersagen von Monte-Carlo-Modellen und den Ergebnissen aus semileptonischen Ereignissen verglichen. …”
Publicado 2001
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20817por Leins, Axel“…Die Daten, bei Schwerpunktsenergien zwischen 189 und 209 GeV, entsprechen einer integrierten Luminositat von ca. 600 pb ¨ 1. …”
Publicado 2002
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20818por Bach, Fabian“…Das u Teilchenspektrum wird dadurch um drei schwere Eichbosonen W ′± und Z ′0 mit Massen zwischen 380 und 600 GeV sowie schwere Fermio- nen mit einer Massenskala von ≳ 3 TeV erweitert. …”
Publicado 2009
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20819por Wood, J. C., Chapman, D. J., Poder, K., Lopes, N. C., Rutherford, M. E., White, T. G., Albert, F., Behm, K. T., Booth, N., Bryant, J. S. J., Foster, P. S., Glenzer, S., Hill, E., Krushelnick, K., Najmudin, Z., Pollock, B. B., Rose, S., Schumaker, W., Scott, R. H. H., Sherlock, M., Thomas, A. G. R., Zhao, Z., Eakins, D. E., Mangles, S. P. D.“…It emanates from a centimetre scale plasma accelerator producing GeV level electron beams. In recent years betatron radiation has been developed as a unique source capable of producing high resolution x-ray images in compact geometries. …”
Publicado 2018
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20820por Liu, Bin, Hinshaw, Robert G., Le, Kevin X., Park, Mi-Ae, Wang, Shuyan, Belanger, Anthony P., Dubey, Shipra, Frost, Jeffrey L., Shi, Qiaoqiao, Holton, Peter, Trojanczyk, Lee, Reiser, Vladimir, Jones, Paul A., Trigg, William, Di Carli, Marcelo F., Lorello, Paul, Caldarone, Barbara J., Williams, Jacqueline P., O’Banion, M. Kerry, Lemere, Cynthia A.“…To investigate the short-term effects of space radiation, we irradiated 4-month-old Alzheimer’s disease (AD)-like transgenic (Tg) mice and wildtype (WT) littermates with a single, whole-body dose of 10 or 50 cGy (56)Fe ions (1 GeV/u) at Brookhaven National Laboratory. At ~1.5 months post irradiation, behavioural testing showed sex-, genotype-, and dose-dependent changes in locomotor activity, contextual fear conditioning, grip strength, and motor learning, mainly in Tg but not WT mice. …”
Publicado 2019
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