Exponential Law of Decay

 

Nearest Star Mass Defect

 

It is important to understand that radioactive decay is entirely a random and unpredictable process.  If we look at any one nucleus, it might decay in ten seconds or ten million years.  There is no way of telling when the decay will happen, and there is certainly no way of speeding up the process.  Remember that chemical reactions involve the outer shell electrons; radioactive decay involves the nucleus.

 

However when we have many millions of millions of nuclei, we can apply statistical models of probability.

 

The rate of disintegration of any nuclide at any time is directly proportional to the number of atoms left at the time:

 

       

This is calculus notation for rate of change in number.

 

The minus sign tells us that N decreases as time increases.

 

There is a constant of proportionality called the radioactive decay constant, which is given the physics code l (greek letter ‘l’, not to be confused with wavelength), and has the units s-1.  So we can write:

 

   

 

The radioactive decay constant is defined as the fraction of the total number of nuclei present that decays per unit time, provided that the time interval is small.  For nuclides with relatively long half-lives, the decay constant will have units “per second”.  However some very unstable nuclides decay in microseconds, so the decay constant would have to be “per nanosecond”.

 

Example

0.25 kg radon-226 emits alpha particles at a measured rate of 9 × 1012 s-1.  What is the decay constant of radium?  (No of atoms in a mole = 6 × 1023)

Work out the number of particles:

0.250 × 6 × 1023 = 6.64 × 1023 atoms

0.226

We know that the rate of decay is 9 × 1012 s-1.  So we use DN/Dt = -lN

                        - 9 × 1012 s-1 = -l × 6.64 × 1023

l = 1.36 × 10-11 s-1

(The minus sign indicates a decay)

 

The unit Becquerel (Bq) is often used.  1 Bq = 1 count per second.

 

 

Over longer periods of time, the relationship above does not hold.  It can be shown by calculus methods (which you are not expected to know), that the decay follows the relationship:

 

 

[N – no of nuclei; N0 – original number of nuclei; e – exponential number, 2.718…; l - decay constant (s-1); t – time (s)]

 

This relationship is described as an exponential decay and the graph looks like this:

 

 

We should note the following:

 

Notice that the horizontal axis is calibrated in periods of time in which the decay goes from an initial value to half that value.  This period is called the half-life.  The formal definition of half-life is the time taken for the activity of a sample to decrease to half some initial value.  After 1 half life the activity is 50 %, between 1 and 2 half lives it falls from 50 % to 25 % and so on.  If we have a whole number of half-lives, we can do an iterative calculation of the fraction remaining, i.e. ½, ¼, 1/8, etc.

 

We can relate the half-life to the decay constant:

 

By definition

 

The formula is N = N0e-lt.  Rearranging gives us

 

T1/2 (pronounced "T-half") is the physics code for half-life.

 

 

This will work for any units of time, although we need to be consistent.

 

To work with these relationships, you must be familiar with the concept of logarithms (a way of expressing a number as a power of 10 or e).  You will see logarithms expressed as ‘lg’ or log10, which means log to the base 10, or ‘ln’ or loge, log to the base e.  The number e is the exponential number, 2.718... The latter is known as natural logarithms, which are at the heart of exponential functions.

 

Example

A radiographer has calculated that a patient is to be injected with 1 ´ 1018 atoms of iodine 131 to monitor thyroid activity.  The half-life is 8 days.  Calculate:

(a)    the radioactive decay constant

(b)   the initial activity

(c)    the number of undecayed atoms of iodine 131 after 24 days.

(d)   The total activity after 3 days.

(a) We need to use T1/2 = 0.693

                                               l

                  we need to convert the 8 days into seconds.

 

                        Þ l =    0.693   _ = 1.00 ´ 10-6 s-1

                                    8 ´ 86400

(b) Use DN = - lN = 1.00 ´ 10-6 s-1 ´ 1 ´ 1018 = 1 ´ 1012 Bq

                Dt

         (c) 24 days is 3 half-lives.  Therefore the number atoms remaining undecayed is 1/8 of the original.

N  =  1 ´ 1018 ¸ 8 = 1.25 ´ 1017

(d) 3 is not so easy.  We use A = A0e-lt

Þ A = 1 ´ 1012 Bq ´ e-(1.00 ´ 10-6 s-1 ´ 3 ´ 86400s)

 

Þ A = 1 ´ 1012 Bq ´ e-(0.2592)

        =  1 ´ 1012 Bq ´ 0.772 = 7.72 ´ 1011 Bq.

[Alternative method] If you are not so confident in the use of the natural logarithm, you can work out the number of half-lives a particular time gives.  In this case 3 days = 3/8 of a half life.

 

Activity = 1 ´ 1012 ´ 1/23/8 = 1 ´ 1012 ´ 1/1.30 = 7.7 ´ 1011 Bq

 

This is a perfectly valid alternative approach.

 

 

The half-life has important implications for the storage of radioactive waste.  Radioactive waste is some of the nastiest muck known to man, so it has to be stored carefully.  Isotopes with a short half-life have intense activities, whereas those with a long half-life have lower activities, but it takes much longer for the activity to decay to a reasonable level.  Either way, it’s not very nice.

 

Even when there have been several half-lives, there remains quite a considerable activity.  If in our example above the activity had decayed to 1/1000th of its original value, we would still have 109 disintegrations per second, which is quite a lot.

 

Another use of the decay equations is in radioactive dating.  Isotopes used are carbon-14, rubidium-87, and hydrogen 3.

 

 

Summary

 

Radioactive decays are random.

 

Rate of decay depends on the number of atoms left

 

The probability of any one nucleus decaying in any one second is the decay constant

 

Decay constant is given the code l

 

DN = -lN

Dt

 

Over a longer period of time, decay is exponential.

 

N = No e-lt

 

Half life is the time taken for ½ the remaining atoms to decay

 

T1/2 = 0.693

              l

 

 

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