GALLEX solar neutrino observations: Results for GALLEX III

CUORE: a cryogenic underground observatory for rare events

“…It is related to the quantity Ω ν , the fraction of the critical density, ρ 0 (that would close the universe) that is in the form of neutrinos, where: Σ = (93.8 eV ) Ω ν h 2 (12) and h is the dimensionless Hubble constant. It was shown in reference [59] that Σ obeys the following inequality with respect to | < m ν > |:…”

“…Suppose we consider the observed neutrino oscillations in the data from atmospheric neutrinos [11] and solar neutrinos [12]. These, coupled with the recent exciting results reported by the Sudbury Neutrino Observatory (SNO) Collaboration [13], gives clear evidence that solar neutrinos oscillate, and that the standard solar model is correct, but that solar electron neutrinos are oscillating to other flavors on their way from the sun, or in the sun.…”

Preliminary Measurement of Neutrino Oscillation Parameters By NuMI/MINOS and Calibration Studies for Improving this Measurement

“…Subsequent experiments used different detector methods in order to try to confirm Davis' measurement. Experiments which detect neutrinos using , such as SAGE [10], GNO [11] and GALLEX [12] did so via the reaction (2.37) and have a relatively low energy threshold of ! .…”

CUORE: The Cryogenic Underground Observatory for Rare Events

“…In addition, neutrino oscillation experiments have yielded the following values of |U ek | 2 : |U e1 | 2 = (0.75 +0.07 −0.12 ), |U e2 | 2 = (0.25 +0. 12 −0.07 ), and |U e3 | 2 = (< 0.026) with confidence levels of 3 σ.…”