Nuclear Stability Calculations

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SUMMARY

This discussion focuses on the equations and principles governing nuclear stability against beta decay, emphasizing the semi-empirical mass formula as a key tool for approximating stability and half-lives of isotopes. It highlights the complexity of deriving nuclear energies from first principles due to the involvement of multiple nucleons and the necessity of accurate nuclear-structure models. The conversation also notes that beta decay half-lives are sensitive to the structure of nuclear states and phase-space factors, making them model-dependent. Overall, understanding these factors is crucial for predicting beta decay behaviors in various isotopes.

PREREQUISITES
  • Familiarity with the semi-empirical mass formula
  • Understanding of nuclear structure models
  • Knowledge of beta decay processes
  • Basic principles of strong interactions in nuclear physics
NEXT STEPS
  • Study the semi-empirical mass formula in detail
  • Research nuclear structure models and their applications
  • Explore the phase-space factors affecting beta decay
  • Investigate publications on theoretical calculations of beta decay half-lives
USEFUL FOR

Nuclear physicists, researchers in nuclear stability, and students studying nuclear decay processes will benefit from this discussion.

gildomar
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Are there equations that detail the stability of nuclei against beta decay? On a related point, I'm familiar with the chart that shows all the isotopes and their half-lives (with a good chunk undergoing beta decay), but I was wondering if that can be derived from first principles, just using the various laws and nucleon counts? And would it cover the likelihood of proton and neutron emission as well? Because I saw that those occur at the some of the extreme edges of the table.
 
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The semi-empirical mass formula gives a good approximation for a large range of nuclei.

Deriving nuclear energies of heavier nuclei from first principles is an extremely challenging task as there are many nucleons involved.

Proton and neutron emission is a process of the strong interaction, if it is energetically "reasonable" it is usually the faster process, but it needs large differences in binding energies.
 
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Thanks! I had somehow managed to forget about that formula. :P

mfb said:
Deriving nuclear energies of heavier nuclei from first principles is an extremely challenging task as there are many nucleons involved.

So that's what would be needed to do in order to help determine what the beta decay half-lives theoretically should be?
 
gildomar said:
Thanks! I had somehow managed to forget about that formula. :P
So that's what would be needed to do in order to help determine what the beta decay half-lives theoretically should be?

Beta decays are very sensitive to structure of the nuclear states which are involved. Therefore, one needs good nuclear-structure models. In addition the half-life depends on the phase-space factor (i.e. the kinematics). The semi-emperical mass formula can tell you whether a nucleus is stable against beta decay. But, the computed half-life is except for the simplest cases quite model dependent.
 
gildomar said:
So that's what would be needed to do in order to help determine what the beta decay half-lives theoretically should be?
The simple model, and then some additional effects like the nuclear shell structure. I'm not a nuclear physics expert, but I know those calculations are done, and there are publications describing how.
 

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