In the upper atmosphere, high-energy cosmic ray neutrons collide with nitrogen-14 nuclei to produce carbon-14, which is vital for radiocarbon dating. The reaction is represented by the equation:
01n+714N→614C+Y {}^{1}_{0}\text{n} + {}^{14}_{7}\text{N} \rightarrow {}^{14}_{6}\text{C} + \text{Y} 01n+714N→614C+YWhat is particle Y\text{Y}Y?
positron
electron
neutron
proton
