The number of radioactive nuclei N(t) at a given time t is given by:
N(t) = N0 \(\times\)exp(-λt)
The activity A of a radioactive source is defined as the rate of decay, which is the derivative of the number of radioactive nuclei with respect to time: A = -\(\frac {dN}{dt}\) = λ\(\times\) N(t)
Given that the activities of sources S1 and S2 are A1 and A2, respectively, we can write:
A1 = λ1 \(\times\) N1(t)
A2 = λ2 \(\times\) N2(t)
After the completion of the 3rd half-life for source S1, the remaining number of radioactive nuclei is:
N1(t) = N0 \(\times\) (\(\frac{1}{2}\))3 = N0 \(\times\) \(\frac {1}{8}\)
Similarly, after the completion of the 7th half-life for source S2, the remaining number of radioactive nuclei is:
N2(t) = N0 \(\times\) \([\frac{1}{2}]\)7 = N0 \(\times\) \(\frac {1}{128}\)
Now, let's substitute these values into the equations for activities A1 and A2 :
A1 = λ1 \(\times\) N0 \(\times\) (\(\frac {1}{8}\))
A2 = λ2 \(\times\) N0 \(\times\) (\(\frac {1}{128}\))
To find the ratio \(\frac{A_1}{A_2}\), we can simplify:
(\(\frac{A_1}{A_2}\)) = (\(\frac{\lambda_1}{\lambda_2}\)) \(\times\) (\(\frac {1}{8}\) ) \(\times\) (\(\frac {128}{1}\))
Since both sources have the same activity at time t = 0, we can assume their decay constants are the same (λ1 = λ2). Therefore, the ratio simplifies to:
(\(\frac{A_1}{A_2}\)) = \(\frac {1}{8}\) \(\times\) \(\frac {128}{1}\) = \(\frac {128}{8}\) = 16
Therefore, the ratio \(\frac{A_1}{A_2}\) is 16.
So, the answer is \(16\).
Nuclear physics is the field of physics that studies atomic nuclei and their constituents and interactions, in addition to the study of other forms of nuclear matter. Nuclear physics should not be confused with atomic physics, which studies the atom as a whole, including its electrons
‘R’ represents the radius of the nucleus. R = RoA1/3
Where,
The mass number (A), also known as the nucleon number, is the total number of neutrons and protons in a nucleus.
A = Z + N
Where, N is the neutron number, A is the mass number, Z is the proton number
Mass defect is the difference between the sum of masses of the nucleons (neutrons + protons) constituting a nucleus and the rest mass of the nucleus and is given as:
Δm = Zmp + (A - Z) mn - M
Where Z = atomic number, A = mass number, mp = mass of 1 proton, mn = mass of 1 neutron and M = mass of nucleus.