binding energy
energy required to separate all the nucleons of a nucleus to infinity
nuclear fusion
2 light nuclei combine to form a heavier nucleus
nuclear fission
a heavy nuclei breaks into 2 smaller nuclei of approximately the same mass
binding energy per nucleon
total energy needed to completely separate all nucleons divided by the number of nucleons in the nucleus
mass defect
difference between total mass of the separate nucleons and combined mass of nucleons
half life
time taken for a radioactive quantity to decrease to half its initial value
radioactive decay
spontaneous and random disintegration of an unstable atomic nucleus