Low-energy-threshold analysis of the Phase I and Phase II data sets of the Sudbury Neutrino Observatory

By J. Monroe, J. Formaggio, M. Miller, B. Monreal, R. Ott, T. Sonley. 2010

213 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/60fd76a22ebe332353ac66f98d48eca6ad7e1fb9

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Citations in the corpus

• Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume II: DUNE Physics (2020, methodology): “The complete data set used, as well as the parameters to which they are sensitive, are (1) from solar neutrino data [298, 413, 414, 415, 416, 417, 418, 419, 420, 421]: θ12, ∆m(2)21, and θ13; (2) from neutrino mode in long-baseline experiments K2K [422], MINOS [423, 424], T2K [425, 426], and NOνA [42”
• Updated global fit to three neutrino mixing: status of the hints of θ13 > 0 (2010, methodology): “kande phase I (SK-I) energy-zenith spectrum [17] and the data from the three phases of SNO [18{20], including the results on the low energy threshold analysis of the combined SNO phase I and phase II [21] (which we label SNO-LETA). We also include the main set of the 192 days of Borexino data [22] (”
• Neutrino Oscillations and Non-standard Interactions (2017, methodology): “SNO took data during three phases, each of them characterized by a different way of detecting the neutrinos produced in the neutrino NC interaction with the heavy water [49, 50].”
• Solar Neutrinos: Status and Prospects (2012, methodology): “…SNO phases (SNO Collaboration, B. Aharmim et al. 2012) and the collaboration’s low-energy analysis of the data from SNO I and II (SNO Collaboration, B. Aharmim et al. 2010); • Borexino’s achievement of a 5% measurement of the 7Be flux, an initial re- sult for the pep flux, and a limit on the…”
• SOLAR MODELS WITH ACCRETION. I. APPLICATION TO THE SOLAR ABUNDANCE PROBLEM (2011, methodology): “Further success came with the first direct measurement of the total 8B neutrino flux by the SNO Collaboration (Ahmad et al. 2002), which proved to be in excellent agreement with standard solar model (SSM) predictions (Bahcall et al. 2001).”