The ability to accurately determine the rate of this H - 17O fusion reaction provides
nuclear physicists with another key
puzzle piece, alongside direct observations of oxygen elemental and isotopic abundances in stellar atmospheres and in primitive meteorites, to zero in on complete and accurate models of stars.
Results from a new study involving Berkeley Lab scientists could explain a mismatch between predictions and recent measurements of ghostly particles streaming from
nuclear reactors — the so - called «reactor antineutrino anomaly» that has
puzzled physicists since 2011.