Search Results - "Montanino, D"

Global analysis of neutrino masses, mixings, and phases: Entering the era of leptonic CP violation searches by Fogli, G L, Lisi, E, Marrone, A, Montanino, D, Palazzo, A, Rotunno, A M

“…We perform a global analysis of neutrino oscillation data, including high-precision measurements of the neutrino mixing angle at reactor experiments, which…”
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Getting the most from the statistical analysis of solar neutrino oscillations by Fogli, G. L., Lisi, E., Marrone, A., Montanino, D., Palazzo, A.

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Probing possible decoherence effects in atmospheric neutrino oscillations by Lisi, E, Marrone, A, Montanino, D

“…It is shown that the results of the Super-Kamiokande atmospheric neutrino experiment, interpreted in terms of nu(mu)<-->nu(tau) flavor transitions, can probe…”
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Analysis of energy and time dependence of supernova shock effects on neutrino crossing probabilities by Fogli, G. L., Lisi, E., Mirizzi, A., Montanino, D.

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Model-dependent and -independent implications of the first Sudbury Neutrino Observatory results by Fogli, G. L., Lisi, E., Montanino, D., Palazzo, A.

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Status of three-neutrino oscillation parameters, circa 2013 by Capozzi, F., Fogli, G. L., Lisi, E., Marrone, A., Montanino, D., Palazzo, A.

“…The standard three-neutrino (3[nu]) oscillation framework is being increasingly refined by results coming from different sets of experiments, using neutrinos…”
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Solar neutrino oscillation parameters after first KamLAND results by Fogli, G. L., Lisi, E., Marrone, A., Montanino, D., Palazzo, A., Rotunno, A. M.

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Three-flavor MSW solutions of the solar neutrino problem by Fogli, G. L., Lisi, E., Montanino, D., Palazzo, A.

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Reexamining nonstandard interaction effects on supernova neutrino flavor oscillations by Fogli, G. L., Lisi, E., Mirizzi, A., Montanino, D.

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Earth regeneration effect in solar neutrino oscillations: An analytic approach by Lisi, Eligio, Montanino, Daniele

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Neutrino masses and mixings: Status of known and unknown 3ν parameters by Capozzi, F., Lisi, E., Marrone, A., Montanino, D., Palazzo, A.

“…Within the standard 3ν mass–mixing framework, we present an up-to-date global analysis of neutrino oscillation data (as of January 2016), including the latest…”
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How to observe 8B solar neutrinos in liquid scintillator detectors by Ianni, A., Montanino, D., Villante, F.L.

“…We show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure the 8B solar neutrino flux by means of the νe charged current…”
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Three-flavor atmospheric neutrino anomaly by Fogli, G. L., Lisi, E., Montanino, D., Scioscia, G.

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Damping of neutrino flavour conversions in a 'noisy' supernova shock-wave by Fogli, G L, Lisi, E, Mirizzi, A, Montanino, D

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Test of non-standard neutrino properties with the BOREXINO source experiments by Ianni, A., Montanino, D., Scioscia, G.

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Test of non-standard neutrino properties with the BOREXINO source experiments by Ianni, A., Montanino, D., Scioscia, G.

“…We calculate the event rates induced by high-intensity radioactive sources of \(\nu_e\) (\(^{51}\)Cr) and of \(\bar{\nu}_e\) (\(^{90}\)Sr), to be located near…”
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The solar neutrino problem after three hundred days of data at SuperKamiokande by Fogli, G.L., Lisi, E., Montanino, D.

“…We present an updated analysis of solar neutrino problem in terms of both Mikheyev-Smirnov-Wolfenstein (MSW) and vacuum neutrino oscillations, with the…”
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Reconciling solar and terrestrial neutrino oscillation evidence with minimum sacrifice by Fogli, G. L., Lisi, E., Montanino, D., Scioscia, G.

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Zenith distribution of atmospheric neutrino events and electron neutrino mixing by Fogli, G.L., Lisi, E., Marrone, A., Montanino, D.

“…Assuming atmospheric neutrino oscillations with dominant ν μ ↔ ν τ transitions, we discuss how subdominant ν e mixing (within the Chooz reactor bounds) can…”
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Discriminating MSW solutions to the solar neutrino problem with flux-independent information at SuperKamiokande and SNO by Fogli, G.L., Lisi, E., Montanino, D.

“…The two possible Mikheyev–Smirnov–Wolfenstein (MSW) solutions of the solar neutrino problem (one at small and the other at large mixing angle), up to now…”
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