The Russian-American Gallium Experiment (SAGE) Cr Neutrino Source Measurement

Abstract

The Russian-American gallium experiment (SAGE) Cr neutrino source measurementhttp://sro.sussex.ac.uk Wark, David and et al, (1996) The Russian-American gallium experiment (SAGE) Cr neutrino source measurement. Physical Review Letters, 77. pp. 4708-4711.

Inertial effects on neutrino oscillations

“…Such results have been found in different experiments: 1) solar neutrino experiments [22,23,24,25,26], 2) atmospheric neutrino experiments [27,28,29,30,31], and 3) the accelerator LSND experiment [32]. Nevertheless, we have to note that many other neutrino oscillation experiments with neutrinos produced by reactors and accelerators did not find any evidence of neutrino oscillations.…”

Reactor antineutrino anomaly with knownθ13

“…The result reported in Ref. [17] included the Gallium neutrino data [19][20][21][22][23][24][25], which was not included in our reactor antineutrino analysis. They also did an analysis by including a RENO preliminary result from the absolute flux analysis.…”

Four-neutrino mixing and Big-Bang Nucleosynthesis

“…Many experiments searching for neutrino oscillations and neutrinoless double-beta decay and investigating the high-energy part of the tritium beta-spectrum are going on or are under preparation. At present, indications that neutrinos are massive and mixed have been found in solar neutrino experiments (Homestake [5], Kamiokande [6], GALLEX [7], SAGE [8] and Super-Kamiokande [9,10]), in atmospheric neutrino experiments (Kamiokande [11], IMB [12], Soudan [13] and Super-Kamiokande [14,10]) and in the LSND experiment [15]. From the analyses of the data of these experiments in terms of neutrino oscillations it follows that there are three different scales of neutrino mass-squared differences: ∆m 2 sun ∼ 10 −5 eV 2 (MSW) or ∆m 2 sun ∼ 10 −10 eV 2 (vac.…”