How can you model half life decay?
1 Answer
The equation would be:
#[A] = 1/(2^(t"/"t_"1/2"))[A]_0#
Read on to know what it means.
Just focus on the main principle:
The upcoming concentration of reactant
#A# after half-life time#t_"1/2"# becomes half of the current concentration.
So, if we define the current concentration as
#[A]_(n+1) = 1/2[A]_n# #" "\mathbf((1))#
We call the (1) the recursive half-life decay equation for one half-life occurrence, i.e. when
Let's go through another half-life, until we've gone through
Notice how
#[A] = (1/2)(1/2)cdots(1/2)[A]_0#
#= (1/2)^n[A]_0#
Now we have (2), the equation for any number of half-life decays... once we know how many half-lives passed by.
However, (2) can be made more convenient since we know that each half-life takes
#nt_"1/2" = t# #" "\mathbf((3))#
That means
Therefore:
#color(blue)([A] = 1/(2^(t"/"t_"1/2"))[A]_0)# #" "\mathbf((4))#
So, we can use (4) to determine half-lives of any typical radioactive element for which we know
#[A]_0# , the initial concentration, and#[A]# , the upcoming concentration, OR#([A])/[A]_0# , the fraction of the element left after time#t# passes.