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Examination of the calorimetric spectrum to determine the neutrino mass in low-energy electron capture decay
R. G. H. Robertson
The standard kinematic method for determining neutrino mass from the beta decay of tritium or other isotope is to measure the shape of the electron spectrum near the endpoint. It h…
Constraining the Leading Weak Axial Two-body Current by SNO and Super-K
Jiunn-Wei Chen, Karsten M. Heeger, R. G. Hamish Robertson
We analyze the Sudbury Neutrino Observatory (SNO) and Super-Kamiokande (SK) data on charged current (CC), neutral current (NC) and neutrino electron elastic scattering (ES) reactio…
Solar Neutrino Interactions with 18O in SuperKamiokande
W. C. Haxton, R. G. H. Robertson
The ratio of 18O nuclei to electrons in SuperKamiokande is quite small, about 1:5000. However this nucleus provides two unpaired neutrons and a low threshold for solar neutrino abs…
Probability of a Solution to the Solar Neutrino Problem Within the Minimal Standard Model
Karsten M. Heeger, R. G. H. Robertson
Tests, independent of any solar model, can be made of whether solar neutrino experiments are consistent with the minimal Standard Model (stable, massless neutrinos). If the experim…