Half-Life Formula: Is It Possible?

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SUMMARY

The discussion centers on the predictability of atomic half-lives based on known values such as the number of protons and neutrons. It confirms that while a definitive formula does not exist, concepts like Fermi's Golden Rule and the Fermi integral (f(Z, E)) provide foundational insights into beta decay. Additionally, the Geiger-Nuttall law establishes a linear relationship between the natural logarithm of half-life and decay energy for alpha decays. These methods serve as initial approximations, with the potential for refinement through advanced theoretical models.

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  • Knowledge of beta and alpha decay processes
  • Familiarity with the Geiger-Nuttall law
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  • Study the applications of Fermi's integral in nuclear physics
  • Explore comparative lifetimes of beta emitters
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pantheid
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Hi, I have always wondered, is there a known formula that predicts the half life of an atom based on known values (e.g., number of protons and neutrons) rather than observation?
 
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Yes - sort of.
The theory predicts the decay crossections for different modes using the initial and final states of the nucleons.
As a starting point, look up: "Fermi's Golden Rule".
 
pantheid said:
Hi, I have always wondered, is there a known formula that predicts the half life of an atom based on known values (e.g., number of protons and neutrons) rather than observation?
The half-life of an atom? You mean the half-life of a nucleus, I assume. Naturally a full answer to this question gets very complex, taking up much of a semester course in nuclear physics. Here's the simplest possible answer: it depends primarily on the energy available for the decay.

For beta decay we utilize a function f(Z, E) called the Fermi integral, and in place of the half-life t1/2 of beta emitters, we study their "comparative lifetimes" ft1/2. We find that ft values are somewhat the same, and fall into several groups depending on whether the decay is "allowed", "superallowed", "forbidden", etc.

For alpha decays, the variation of ln(t1/2) versus decay energy results in a linear relation, the Geiger-Nuttall law.

In both cases these results are just first approximations, which can be improved by more detailed theoretical models.
 

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