Stellar Physics 5b: Nuclear Stability
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Qualitative overview of the criteria for nuclear stability, based on the Semi-Empirical Mass Formula. This video directly follows material from Stellar Physics 5a. it covers:
- Review of the Semi-Empirical Mass Formula (derived in Stellar Physics 5a)
- Valley of beta-stability
- Criteria for nuclear stability/decay
- Nuclear decay modes
- Nuclear binding energy per nucleon
- Review of the Semi-Empirical Mass Formula (derived in Stellar Physics 5a)
- Valley of beta-stability
- Criteria for nuclear stability/decay
- Nuclear decay modes
- Nuclear binding energy per nucleon
