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Wyszukujesz frazę "Hungerford, E." wg kryterium: Autor


Tytuł:
SOX : short distance neutrino Oscillations with BoreXino
Autorzy:
Miramonti, L.
Franco, D.
Cavalcante, P.
Ianni, Andrea
Unzhakov, E.
Bick, D.
Mosteiro, P.
Goretti, A.
Lombardi, P.
Otis, K.
Sotnikov, A.
Link, J. M.
Korga, G.
Salvo, C.
Suvorov, Y.
Perasso, S.
Chavarria, A.
Hungerford, E.
Fernandes, G.
Misiaszek, Marcin
Razeto, A.
Sukhotin, S.
Manecki, S.
Pallavicini, M.
Wurm, M.
Bellini, G.
Romani, A.
Korablev, D.
Kobychev, V.
Kryn, D.
Meyer, M.
Wang, H.
Semenov, D.
Ortica, F.
Hagner, C.
Skorokhvatov, M.
Zuzel, Grzegorz
Bravo, D.
Simgen, H.
Ranucci, G.
Re, A.
Davini, S.
Tartaglia, R.
Caminata, A.
Caccianiga, B.
Oberauer, L.
Vogelaar, R. B.
Etenko, A.
Chepurnov, A.
Ghiano, C.
Schönert, S.
Pocar, A.
Papp, L.
Saldanha, R.
Testera, G.
Zavatarelli, S.
Lombardi, F.
Lukyanchenko, G.
Meroni, E.
Ludhova, L.
Bonfini, G.
Laubenstein, M.
Göger-Neff, M.
Smirnov, O.
Obolensky, M.
Calaprice, F.
Pantic, E.
Krasnicky, D.
Machulin, I.
Zaimidoroga, O.
Ianni, Aldo
Fomenko, K.
Rossi, N.
D’Angelo, D.
Derbin, A.
Muratova, V.
Galbiati, C.
Maneschg, W.
Wójcik, Marcin
Litvinovich, E.
Opis:
The very low radioactive background of the Borexino detector, its large size, and the well proved capability to detect both low energy electron neutrinos and antineutrinos make an ideal case for the study of short distance neutrino oscillations with artificial sources at Gran Sasso. This paper describes the possible layouts of $^{51}Cr(v_{e})$ and $^{144}Ce-^{144}Pr(\bar{v}_{e})$ source experiments in Borexino and shows the expected sensitivity to eV mass sterile neutrinos for three possible different phases of the experiment. Expected results on neutrino magnetic moment, electroweak mixing angle, and couplings to axial and vector currents are shown too.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Short distance neutrino oscillations with BoreXino : SOX
Autorzy:
Miramonti, L.
Franco, D.
Cavalcante, P.
Ianni, Andrea
Winter, J.
Bick, D.
Lehnert, B.
Mosteiro, P.
Goretti, A.
Lombardi, P.
Otis, K.
Sotnikov, A.
Korga, G.
Salvo, C.
Suvorov, Y.
Hungerford, E.
Misiaszek, Marcin
Razeto, A.
Zuber, K.
Sukhotin, S.
Manecki, S.
Pallavicini, M.
Wurm, M.
Bellini, G.
Romani, A.
Korablev, D.
Kobychev, V.
Kryn, D.
Lewke, T.
Meyer, M.
Wang, H.
Marcocci, S.
Ortica, F.
Hagner, C.
Skorokhvatov, M.
Zuzel, Grzegorz
Bravo, D.
Simgen, H.
Ranucci, G.
Re, A.
Davini, S.
Empl, A.
Vignaud, D.
Tartaglia, R.
Wright, A.
Caminata, A.
Caccianiga, B.
Oberauer, L.
Vogelaar, R. B.
Etenko, A.
Perasso, L.
Chepurnov, A.
Benziger, J.
Ghiano, C.
Schönert, S.
Pocar, A.
Papp, L.
von Feilitzsch, F.
Meindl, Q.
Saldanha, R.
Testera, G.
Zavatarelli, S.
Lombardi, F.
Lukyanchenko, G.
Meroni, E.
Ludhova, L.
Bonfini, G.
Laubenstein, M.
Göger-Neff, M.
Smirnov, O.
Obolensky, M.
Wójcik, Marcin
Calaprice, F.
Machulin, I.
Zaimidoroga, O.
Ianni, Aldo
Giammarchi, M.
Fomenko, K.
Rossi, N.
D’Angelo, D.
Derbin, A.
Muratova, V.
Gazzana, S.
Galbiati, C.
Maneschg, W.
Chavarria, A.
Litvinovich, E.
Opis:
Borexino, a large volume liquid scintillator detector installed at Gran Sasso laboratory, demonstrated extraordinary sensitivity with respect to neutrino and antineutrino detection, reporting the best up to date results on low energy solar neutrino fluxes and performing geo-neutrino detection. Energy and position of 1 MeV events in Borexino are recon- structed with a precision of 5% and 14 cm respectively. These performances together with extremely low background provides an excellent opportunity for the study of short distance neutrino oscillations on the eV mass scale with artificial neutrino sources. The possible layouts for 51Cr (monoenergetic neutrino) and 144Ce–144Pr (antineutrino from β-decay) source experiments in Borexino and the expected sensitivity to sterile neutrinos for three possible designs of the experiment are presented.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Real-time detection of solar neutrinos with Borexino
Autorzy:
Laubenstein, M.
Pallavicini, M.
Tartaglia, R.
Bonfini, G.
Yokley, Z.
Wójcik, Marcin
Meyer, M.
Caminata, A.
Rossi, N.
Papp, L.
Agostini, M.
Fomenko, K.
Zavatarelli, S.
Razeto, A.
Di, Noto
Suvorov, Y.
Re, A.
Ludhova, L.
Bick, D.
Winter, J.
Caccianiga, B.
Toropova, M.
Benziger, J.
Sukhotin, S.
Carlini, M.
Appel, S.
Kryn, D.
Montuschi, M.
Skorokhvatov, M.
Meroni, E.
Unzhakov, E.
Wurm, M.
Vishneva, A.
Formozov, A.
Altenmüller, K.
Franco, D.
Perasso, L.
Manecki, S.
Bravo, D.
Wang, H.
Miramonti, L.
Ianni, A.
Ortica, F.
Simgen, H.
Schönert, S.
Giammarchi, M.
Ranucci, G.
Gabriele, F.
Litvinovich, E.
Marcocci, S.
Cavalcante, P.
Goeger-Neff, M.
Ghiano, C.
Gromov, M.
Romani, A.
Korablev, D.
Goretti, A.
Chepurnov, A.
Etenko, A.
Kaiser, M.
Pocar, A.
Oberauer, L.
Thurn, J.
D'Angelo, D.
Lehnert, B.
Jeschke, D.
Derbin, A.
Galbiati, C.
Calaprice, F.
Davini, S.
Neumair, B.
Zaimidoroga, O.
Hagner, C.
Testera, G.
Misiaszek, Marcin
Kobychev, V.
Korga, G.
Semenov, D.
Muratova, V.
Roncin, R.
Machulin, I.
Sotnikov, A.
Hungerford, E.
Weinz, S.
Jędrzejczak, Karol
Drachnev, I.
Bellini, G.
Von, Feilitzsch
Smirnov, O.
Zuzel, Grzegorz
Maneschg, W.
Obolensky, M.
Lukyanchenko, G.
Mosteiro, P.
Vogelaar, R. B.
Lombardi, F.
Zuber, K.
Lombardi, P.
Opis:
Solar neutrinos have been fundamental in the discovery of neutrino flavor oscillations and are a unique tool to probe the nuclear reactions that fuel the Sun. The Borexino experiment, located in the Gran Sasso National Laboratory, is an ultra-pure liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos. Thanks to its unprecedented background levels, Borexino could measure in real time the fluxes of different components of the solar neutrino spectrum, thus probing both solar neutrino oscillations and the Standard Solar Model. We review these fundamental results and also discuss the prospects for the Phase-II of Borexino, which is entering the precision era of solar neutrino measurements.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Artykuł
Tytuł:
Overview and accomplishments of the Borexino experiment
Autorzy:
Miramonti, L.
Franco, D.
Drachnev, I.
Roncin, R.
Cavalcante, P.
Ianni, Andrea
Winter, J.
Unzhakov, E.
Bick, D.
Lehnert, B.
Mosteiro, P.
Kaiser, M.
Goretti, A.
Lombardi, P.
Sotnikov, A.
Korga, G.
Noto, L. Di
Suvorov, Y.
Vishneva, A.
Hungerford, E.
Neumair, B.
Weinz, S.
Misiaszek, Marcin
Razeto, A.
Zuber, K.
Sukhotin, S.
Manecki, S.
Pallavicini, M.
Wurm, M.
Bellini, G.
Romani, A.
Korablev, D.
Kobychev, V.
Kryn, D.
Meyer, M.
Wang, H.
Marcocci, S.
Semenov, D.
Ortica, F.
Hagner, C.
Skorokhvatov, M.
Zuzel, Grzegorz
Bravo, D.
Agostini, M.
Simgen, H.
Gromov, M.
Ranucci, G.
Re, A.
Yokley, Z.
Davini, S.
Gabriele, F.
Tartaglia, R.
Caminata, A.
Caccianiga, B.
Oberauer, L.
Vogelaar, R. B.
Etenko, A.
Montuschi, M.
Jędrzejczak, Karol
Perasso, L.
Chepurnov, A.
Benziger, J.
Ghiano, C.
Schönert, S.
Pocar, A.
Papp, L.
Testera, G.
Zavatarelli, S.
Lombardi, F.
Goeger-Neff, M.
Lukyanchenko, G.
Meroni, E.
Appel, S.
Ludhova, L.
Bonfini, G.
D'Angelo, D.
Feilitzsch, F. von
Laubenstein, M.
Smirnov, O.
Obolensky, M.
Calaprice, F.
Machulin, I.
Thurn, J.
Zaimidoroga, O.
Ianni, Aldo
Giammarchi, M.
Fomenko, K.
Rossi, N.
Derbin, A.
Muratova, V.
Galbiati, C.
Toropova, M.
Maneschg, W.
Wójcik, Marcin
Litvinovich, E.
Opis:
The Borexino experiment is running at the Laboratori del Gran Sasso in Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the basis of the outstanding achievements accumulated by the experiment. In this talk, after recalling the main features of the detector, the impressive solar data gathered so far by the experiment will be summarized, with special emphasis to the most recent and prominent result concerning the detection of the fundamental pp solar neutrino flux, which is the direct probe of the engine mechanism powering our star. Such a milestone measurement puts Borexino in the unique situation of being the only experiment able to do solar neutrino spectroscopy over the entire solar spectrum; the counterpart of this peculiar status in the oscillation interpretation of the data is the capability of Borexino alone to perform the full validation across the solar energy range of the MSW-LMA paradigm. The talk will be concluded highlighting the perspectives for the final stage of the solar program of the experiment, centered on the goal to fully complete the solar spectroscopy with the missing piece of the CNO neutrinos. If successful, such a measurement would represent the final crowning of the long quest of Borexino to unravel all the properties of the neutrinos from the Sun.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Inne
Tytuł:
Measurement of Solar pp-neutrino flux with Borexino : results and implications
Autorzy:
Miramonti, L.
Franco, D.
Drachnev, I.
Roncin, R.
Cavalcante, P.
Ianni, Andrea
Winter, J.
Unzhakov, E.
Bick, D.
Lehnert, B.
Mosteiro, P.
Kaiser, M.
Goretti, A.
Lombardi, P.
Sotnikov, A.
Korga, G.
Noto, L. Di
Suvorov, Y.
Vishneva, A.
Hungerford, E.
Neumair, B.
Weinz, S.
Misiaszek, Marcin
Razeto, A.
Zuber, K.
Sukhotin, S.
Manecki, S.
Pallavicini, M.
Wurm, M.
Bellini, G.
Romani, A.
Korablev, D.
Kobychev, V.
Kryn, D.
Meyer, M.
Wang, H.
Marcocci, S.
Semenov, D.
Ortica, F.
Hagner, C.
Skorokhvatov, M.
Zuzel, Grzegorz
Bravo, D.
Agostini, M.
Simgen, H.
Gromov, M.
Ranucci, G.
Re, A.
Yokley, Z.
Davini, S.
Gabriele, F.
Tartaglia, R.
Caminata, A.
Caccianiga, B.
Oberauer, L.
Vogelaar, R. B.
Etenko, A.
Montuschi, M.
Jędrzejczak, Karol
Perasso, L.
Chepurnov, A.
Benziger, J.
Ghiano, C.
Schönert, S.
Pocar, A.
Papp, L.
Smirnov, O. Yu
Testera, G.
Zavatarelli, S.
Lombardi, F.
Goeger-Neff, M.
Lukyanchenko, G.
Meroni, E.
Appel, S.
Ludhova, L.
Bonfini, G.
D'Angelo, D.
Feilitzsch, F. von
Laubenstein, M.
Obolensky, M.
Calaprice, F.
Thurn, J.
Zaimidoroga, O.
Ianni, Aldo
Giammarchi, M.
Fomenko, K.
Rossi, N.
Derbin, A.
Muratova, V.
Galbiati, C.
Toropova, M.
Machulin, O.
Maneschg, W.
Wójcik, Marcin
Litvinovich, E.
Opis:
Measurement of the Solar pp-neutrino flux completed the measurement of Solar neutrino fluxes from the pp-chain of reactions in Borexino experiment. The result is in agreement with the prediction of the Standard Solar Model and the MSW/LMA oscillation scenario. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10^{5} years time scale, and sets a strong limit on the power production by the unknown energy sources in the Sun.
Dostawca treści:
Repozytorium Uniwersytetu Jagiellońskiego
Inne

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