- Ex 5B Radioactive Decay and Half Life - This should be complete by now
- Ex 5C Nuclear Reactions and Nuclear Energy Calculations - due next week
Nuclear Fusion in the Sun
Binding Energy comes from the change in mass from individual nucleons to being combined into a nucleus. This is energy lost by the nucleons joined together in a nucleus and must be returned in order to separate the nucleons
E = Δmc2
Mass Energy Equivalence
Nuclear Reactions
Fission Fusion and Radioactive Decay
Fission & Fusion
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