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Your search keyword '"Manuzio, G."' showing total 10 results
Start Over Author "Manuzio, G." Journal physical review letters
10 results on '"Manuzio, G."'

1. Direct Measurement of theBe7Solar Neutrino Flux with 192 Days of Borexino Data

Author

Arpesella, C., primary, Back, H. O., additional, Balata, M., additional, Bellini, G., additional, Benziger, J., additional, Bonetti, S., additional, Brigatti, A., additional, Caccianiga, B., additional, Cadonati, L., additional, Calaprice, F., additional, Carraro, C., additional, Cecchet, G., additional, Chavarria, A., additional, Chen, M., additional, Dalnoki-Veress, F., additional, D’Angelo, D., additional, de Bari, A., additional, de Bellefon, A., additional, de Kerret, H., additional, Derbin, A., additional, Deutsch, M., additional, di Credico, A., additional, di Pietro, G., additional, Eisenstein, R., additional, Elisei, F., additional, Etenko, A., additional, Fernholz, R., additional, Fomenko, K., additional, Ford, R., additional, Franco, D., additional, Freudiger, B., additional, Galbiati, C., additional, Gatti, F., additional, Gazzana, S., additional, Giammarchi, M., additional, Giugni, D., additional, Goeger-Neff, M., additional, Goldbrunner, T., additional, Goretti, A., additional, Grieb, C., additional, Hagner, C., additional, Hampel, W., additional, Harding, E., additional, Hardy, S., additional, Hartman, F. X., additional, Hertrich, T., additional, Heusser, G., additional, Ianni, Aldo, additional, Ianni, Andrea, additional, Joyce, M., additional, Kiko, J., additional, Kirsten, T., additional, Kobychev, V., additional, Korga, G., additional, Korschinek, G., additional, Kryn, D., additional, Lagomarsino, V., additional, Lamarche, P., additional, Laubenstein, M., additional, Lendvai, C., additional, Leung, M., additional, Lewke, T., additional, Litvinovich, E., additional, Loer, B., additional, Lombardi, P., additional, Ludhova, L., additional, Machulin, I., additional, Malvezzi, S., additional, Manecki, S., additional, Maneira, J., additional, Maneschg, W., additional, Manno, I., additional, Manuzio, D., additional, Manuzio, G., additional, Martemianov, A., additional, Masetti, F., additional, Mazzucato, U., additional, McCarty, K., additional, McKinsey, D., additional, Meindl, Q., additional, Meroni, E., additional, Miramonti, L., additional, Misiaszek, M., additional, Montanari, D., additional, Monzani, M. E., additional, Muratova, V., additional, Musico, P., additional, Neder, H., additional, Nelson, A., additional, Niedermeier, L., additional, Oberauer, L., additional, Obolensky, M., additional, Orsini, M., additional, Ortica, F., additional, Pallavicini, M., additional, Papp, L., additional, Parmeggiano, S., additional, Perasso, L., additional, Pocar, A., additional, Raghavan, R. S., additional, Ranucci, G., additional, Rau, W., additional, Razeto, A., additional, Resconi, E., additional, Risso, P., additional, Romani, A., additional, Rountree, D., additional, Sabelnikov, A., additional, Saldanha, R., additional, Salvo, C., additional, Schimizzi, D., additional, Schönert, S., additional, Shutt, T., additional, Simgen, H., additional, Skorokhvatov, M., additional, Smirnov, O., additional, Sonnenschein, A., additional, Sotnikov, A., additional, Sukhotin, S., additional, Suvorov, Y., additional, Tartaglia, R., additional, Testera, G., additional, Vignaud, D., additional, Vitale, S., additional, Vogelaar, R. B., additional, von Feilitzsch, F., additional, von Hentig, R., additional, von Hentig, T., additional, Wojcik, M., additional, Wurm, M., additional, Zaimidoroga, O., additional, Zavatarelli, S., additional, and Zuzel, G., additional

Published
2008
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2. Temporally Controlled Modulation of Antihydrogen Production and the Temperature Scaling of Antiproton-Positron Recombination

Author

Fujiwara, M. C., primary, Amoretti, M., additional, Amsler, C., additional, Bonomi, G., additional, Bouchta, A., additional, Bowe, P. D., additional, Canali, C., additional, Carraro, C., additional, Cesar, C. L., additional, Charlton, M., additional, Doser, M., additional, Fontana, A., additional, Funakoshi, R., additional, Genova, P., additional, Hangst, J. S., additional, Hayano, R. S., additional, Jørgensen, L. V., additional, Kellerbauer, A., additional, Lagomarsino, V., additional, Landua, R., additional, Lodi-Rizzini, E., additional, Macri, M., additional, Madsen, N., additional, Manuzio, G., additional, Mitchard, D., additional, Montagna, P., additional, Pruys, H., additional, Regenfus, C., additional, Rotondi, A., additional, Testera, G., additional, Variola, A., additional, Venturelli, L., additional, van der Werf, D. P., additional, Yamazaki, Y., additional, and Zurlo, N., additional

Published
2008
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3. Search for Laser-Induced Formation of Antihydrogen Atoms

Author

Amoretti, M., primary, Amsler, C., additional, Bonomi, G., additional, Bowe, P. D., additional, Canali, C., additional, Carraro, C., additional, Cesar, C. L., additional, Charlton, M., additional, Ejsing, A. M., additional, Fontana, A., additional, Fujiwara, M. C., additional, Funakoshi, R., additional, Genova, P., additional, Hangst, J. S., additional, Hayano, R. S., additional, Jørgensen, L. V., additional, Kellerbauer, A., additional, Lagomarsino, V., additional, Lodi Rizzini, E., additional, Macrì, M., additional, Madsen, N., additional, Manuzio, G., additional, Mitchard, D., additional, Montagna, P., additional, Posada, L. G. C., additional, Pruys, H., additional, Regenfus, C., additional, Rotondi, A., additional, Telle, H. H., additional, Testera, G., additional, Van der Werf, D. P., additional, Variola, A., additional, Venturelli, L., additional, Yamazaki, Y., additional, and Zurlo, N., additional

Published
2006
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4. Evidence For The Production Of Slow Antiprotonic Hydrogen In Vacuum

Author

Zurlo, N., primary, Amoretti, M., additional, Amsler, C., additional, Bonomi, G., additional, Carraro, C., additional, Cesar, C. L., additional, Charlton, M., additional, Doser, M., additional, Fontana, A., additional, Funakoshi, R., additional, Genova, P., additional, Hayano, R. S., additional, Jørgensen, L. V., additional, Kellerbauer, A., additional, Lagomarsino, V., additional, Landua, R., additional, Rizzini, E. Lodi, additional, Macrì, M., additional, Madsen, N., additional, Manuzio, G., additional, Mitchard, D., additional, Montagna, P., additional, Posada, L. G., additional, Pruys, H., additional, Regenfus, C., additional, Rotondi, A., additional, Testera, G., additional, der Werf, D. P. Van, additional, Variola, A., additional, Venturelli, L., additional, and Yamazaki, Y., additional

Published
2006
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5. Three-Dimensional Annihilation Imaging of Trapped Antiprotons

Author

Fujiwara, M. C., primary, Amoretti, M., additional, Bonomi, G., additional, Bouchta, A., additional, Bowe, P. D., additional, Carraro, C., additional, Cesar, C. L., additional, Charlton, M., additional, Doser, M., additional, Filippini, V., additional, Fontana, A., additional, Funakoshi, R., additional, Genova, P., additional, Hangst, J. S., additional, Hayano, R. S., additional, Jørgensen, L. V., additional, Lagomarsino, V., additional, Landua, R., additional, Lodi-Rizzini, E., additional, Marchesotti, M., additional, Macri, M., additional, Madsen, N., additional, Manuzio, G., additional, Montagna, P., additional, Riedler, P., additional, Rotondi, A., additional, Rouleau, G., additional, Testera, G., additional, Variola, A., additional, van der Werf, D. P., additional, and Yamazaki, Y., additional

Published
2004
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6. Positron Plasma Diagnostics and Temperature Control for Antihydrogen Production

Author

Amoretti, M., primary, Amsler, C., additional, Bonomi, G., additional, Bouchta, A., additional, Bowe, P. D., additional, Carraro, C., additional, Cesar, C. L., additional, Charlton, M., additional, Doser, M., additional, Filippini, V., additional, Fontana, A., additional, Fujiwara, M. C., additional, Funakoshi, R., additional, Genova, P., additional, Hangst, J. S., additional, Hayano, R. S., additional, Jørgensen, L. V., additional, Lagomarsino, V., additional, Landua, R., additional, Lindelöf, D., additional, Rizzini, E. Lodi, additional, Macrí, M., additional, Madsen, N., additional, Manuzio, G., additional, Montagna, P., additional, Pruys, H., additional, Regenfus, C., additional, Rotondi, A., additional, Testera, G., additional, Variola, A., additional, and van der Werf, D. P., additional

Published
2003
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8. First evidence of pep solar neutrinos by direct detection in Borexino.

Author

Bellini G, Benziger J, Bick D, Bonetti S, Bonfini G, Bravo D, Buizza Avanzini M, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cavalcante P, Chavarria A, Chepurnov A, D'Angelo D, Davini S, Derbin A, Etenko A, Fomenko K, Franco D, Galbiati C, Gazzana S, Ghiano C, Giammarchi M, Goeger-Neff M, Goretti A, Grandi L, Guardincerri E, Hardy S, Ianni A, Ianni A, Korablev D, Korga G, Koshio Y, Kryn D, Laubenstein M, Lewke T, Litvinovich E, Loer B, Lombardi F, Lombardi P, Ludhova L, Machulin I, Manecki S, Maneschg W, Manuzio G, Meindl Q, Meroni E, Miramonti L, Misiaszek M, Montanari D, Mosteiro P, Muratova V, Oberauer L, Obolensky M, Ortica F, Otis K, Pallavicini M, Papp L, Perasso L, Perasso S, Pocar A, Quirk J, Raghavan RS, Ranucci G, Razeto A, Re A, Romani A, Sabelnikov A, Saldanha R, Salvo C, Schönert S, Simgen H, Skorokhvatov M, Smirnov O, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vogelaar RB, von Feilitzsch F, Winter J, Wojcik M, Wright A, Wurm M, Xu J, Zaimidoroga O, Zavatarelli S, and Zuzel G

Abstract

We observed, for the first time, solar neutrinos in the 1.0-1.5 MeV energy range. We determined the rate of pep solar neutrino interactions in Borexino to be 3.1±0.6{stat}±0.3{syst}  counts/(day·100  ton). Assuming the pep neutrino flux predicted by the standard solar model, we obtained a constraint on the CNO solar neutrino interaction rate of <7.9  counts/(day·100  ton) (95% C.L.). The absence of the solar neutrino signal is disfavored at 99.97% C.L., while the absence of the pep signal is disfavored at 98% C.L. The necessary sensitivity was achieved by adopting data analysis techniques for the rejection of cosmogenic {11}C, the dominant background in the 1-2 MeV region. Assuming the Mikheyev-Smirnov-Wolfenstein large mixing angle solution to solar neutrino oscillations, these values correspond to solar neutrino fluxes of (1.6±0.3)×10{8}  cm{-2} s^{-1} and <7.7×10{8}  cm{-2} s{-1} (95% C.L.), respectively, in agreement with both the high and low metallicity standard solar models. These results represent the first direct evidence of the pep neutrino signal and the strongest constraint of the CNO solar neutrino flux to date.

Published
2012
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9. Precision measurement of the (7)Be solar neutrino interaction rate in Borexino.

Author

Bellini G, Benziger J, Bick D, Bonetti S, Bonfini G, Buizza Avanzini M, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cavalcante P, Chavarria A, D'Angelo D, Davini S, Derbin A, Etenko A, Fomenko K, Franco D, Galbiati C, Gazzana S, Ghiano C, Giammarchi M, Goeger-Neff M, Goretti A, Grandi L, Guardincerri E, Hardy S, Ianni A, Ianni A, Kobychev V, Korablev D, Korga G, Koshio Y, Kryn D, Laubenstein M, Lewke T, Litvinovich E, Loer B, Lombardi F, Lombardi P, Ludhova L, Machulin I, Manecki S, Maneschg W, Manuzio G, Meindl Q, Meroni E, Miramonti L, Misiaszek M, Montanari D, Mosteiro P, Muratova V, Oberauer L, Obolensky M, Ortica F, Pallavicini M, Papp L, Peña-Garay C, Perasso L, Perasso S, Pocar A, Raghavan RS, Ranucci G, Razeto A, Re A, Romani A, Sabelnikov A, Saldanha R, Salvo C, Schönert S, Simgen H, Skorokhvatov M, Smirnov O, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vogelaar RB, von Feilitzsch F, Winter J, Wojcik M, Wright A, Wurm M, Xu J, Zaimidoroga O, Zavatarelli S, and Zuzel G

Abstract

The rate of neutrino-electron elastic scattering interactions from 862 keV (7)Be solar neutrinos in Borexino is determined to be 46.0±1.5(stat)(-1.6)(+1.5)(syst) counts/(day·100  ton). This corresponds to a ν(e)-equivalent (7)Be solar neutrino flux of (3.10±0.15)×10(9)  cm(-2) s(-1) and, under the assumption of ν(e) transition to other active neutrino flavours, yields an electron neutrino survival probability of 0.51±0.07 at 862 keV. The no flavor change hypothesis is ruled out at 5.0 σ. A global solar neutrino analysis with free fluxes determines Φ(pp)=6.06(-0.06)(+0.02)×10(10)  cm(-2) s(-1) and Φ(CNO)<1.3×10(9)  cm(-2) s(-1) (95% C.L.). These results significantly improve the precision with which the Mikheyev-Smirnov-Wolfenstein large mixing angle neutrino oscillation model is experimentally tested at low energy.

Published
2011
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10. Direct measurement of the 7Be solar neutrino flux with 192 days of borexino data.

Author

Arpesella C, Back HO, Balata M, Bellini G, Benziger J, Bonetti S, Brigatti A, Caccianiga B, Cadonati L, Calaprice F, Carraro C, Cecchet G, Chavarria A, Chen M, Dalnoki-Veress F, D'Angelo D, de Bari A, de Bellefon A, de Kerret H, Derbin A, Deutsch M, di Credico A, di Pietro G, Eisenstein R, Elisei F, Etenko A, Fernholz R, Fomenko K, Ford R, Franco D, Freudiger B, Galbiati C, Gatti F, Gazzana S, Giammarchi M, Giugni D, Goeger-Neff M, Goldbrunner T, Goretti A, Grieb C, Hagner C, Hampel W, Harding E, Hardy S, Hartman FX, Hertrich T, Heusser G, Ianni A, Ianni A, Joyce M, Kiko J, Kirsten T, Kobychev V, Korga G, Korschinek G, Kryn D, Lagomarsino V, Lamarche P, Laubenstein M, Lendvai C, Leung M, Lewke T, Litvinovich E, Loer B, Lombardi P, Ludhova L, Machulin I, Malvezzi S, Manecki S, Maneira J, Maneschg W, Manno I, Manuzio D, Manuzio G, Martemianov A, Masetti F, Mazzucato U, McCarty K, McKinsey D, Meindl Q, Meroni E, Miramonti L, Misiaszek M, Montanari D, Monzani ME, Muratova V, Musico P, Neder H, Nelson A, Niedermeier L, Oberauer L, Obolensky M, Orsini M, Ortica F, Pallavicini M, Papp L, Parmeggiano S, Perasso L, Pocar A, Raghavan RS, Ranucci G, Rau W, Razeto A, Resconi E, Risso P, Romani A, Rountree D, Sabelnikov A, Saldanha R, Salvo C, Schimizzi D, Schönert S, Shutt T, Simgen H, Skorokhvatov M, Smirnov O, Sonnenschein A, Sotnikov A, Sukhotin S, Suvorov Y, Tartaglia R, Testera G, Vignaud D, Vitale S, Vogelaar RB, von Feilitzsch F, von Hentig R, von Hentig T, Wojcik M, Wurm M, Zaimidoroga O, Zavatarelli S, and Zuzel G

Abstract

We report the direct measurement of the 7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the 0.862 MeV 7Be neutrinos is 49+/-3stat+/-4syst counts/(day.100 ton). The hypothesis of no oscillation for 7Be solar neutrinos is inconsistent with our measurement at the 4sigma C.L. Our result is the first direct measurement of the survival probability for solar nu(e) in the transition region between matter-enhanced and vacuum-driven oscillations. The measurement improves the experimental determination of the flux of 7Be, pp, and CNO solar nu(e), and the limit on the effective neutrino magnetic moment using solar neutrinos.

Published
2008
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