What is the Process and Mathematical Explanation of Radioactive Decay?

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SUMMARY

Radioactive decay is the process where an unstable atomic nucleus emits radiation, transforming from a parent nuclide to a daughter nuclide. The activity (A) of a radioactive sample is proportional to the number of radioactive nuclei (N), expressed mathematically as A = -dN/dt = λN, where λ is the decay constant. The solution to this equation is A = A₀e^{-λt}, indicating how activity decreases over time. Similarly, the remaining number of nuclei is given by N = N₀e^{-λt}, illustrating the exponential nature of decay.

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Definition/Summary

Radioactive decay is the process in which an unstable atomic nucleus loses energy by emitting radiation in the form of particles or electromagnetic waves. This decay, or loss of energy, results in an atom of one type, called the parent nuclide transforming to an atom of a different type, called the daughter nuclide.


Equations

The activity (A) of a radioactive sample (the number of decays per unit time) is found to be proportional to the number of radioactive nuclei (N) in a given sample. That is,

A = - \frac{dN}{dt} = \lambda N

Where \lambda is the constant of proportionality and is called the decay constant. The above expression is a separable ODE and has a solution,

A = A_0e^{-\lambda t}

Where A_0 represents the initial activity of the sample at t=0. Equivalently, one can form an expression for the number of remaining radioactive nuclei,

N = N_0e^{-\lambda t}

Where N_0 represents the initial number of radioactive nuclei at t=0.

Extended explanation



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Thanks for the explanation. This is a great way to understand radioactive decay and the equations associated with it.
 

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