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"It's ironic: in order to observe the Sun, you need to go kilometers underground." -Art McDonald
Imagine you finally thought you understood how the Sun worked: how light elements fused into heavier ones, emitting energy in the process. And when you finally completed your calculations, you got nuclear physics results that matched what you observed exactly, energy outputs that fit, and a prediction for the emission of neutrinos.
This guest post is by Brookhaven Lab physicist Steve Kettell, the Chief Scientist for the U.S. Daya Bay Neutrino Project in southern China. Kettell received his Ph.D. in 1990 from Yale University and is the leader of Brookhaven's Electronic Detector Group.