SUMMARY
The necessary conditions for a nucleus to undergo fission with a thermal neutron include the absorption of the neutron by a fissile nucleus, which is typically characterized by a low activation energy, a mass number greater than 210, and a specific neutron-to-proton ratio (N/Z). Fissile isotopes such as U-233, U-235, Pu-239, and Pu-241 are known to readily undergo fission upon thermal neutron absorption. Upon absorption, there is an approximately 84% probability of fission occurring, while a 16% chance exists for gamma decay, resulting in the formation of an excited state nucleus. The pairing term in the semi-empirical mass formula plays a significant role in determining the likelihood of fission for even N nuclei.
PREREQUISITES
- Understanding of nuclear fission principles
- Familiarity with thermal neutron interactions
- Knowledge of isotopes, specifically U and Pu
- Basic grasp of the semi-empirical mass formula
NEXT STEPS
- Research the neutron energy-dependent cross sections for fission reactions
- Study the semi-empirical mass formula and its implications for nuclear stability
- Examine the binding energy per nucleon for isotopes of U and Pu
- Explore the differences between even-even, odd-odd, and even-odd nuclei in fission processes
USEFUL FOR
Students and professionals in nuclear physics, nuclear engineers, and researchers focusing on nuclear fission and reactor design will benefit from this discussion.