In a nuclear fission reaction of an isotope of mass \( M \), three similar daughter nuclei of the same mass are formed. The speed of a daughter nuclei in terms of mass defect \( \Delta M \) will be:
\( c \sqrt{\frac{c \Delta M}{M}} \)
\( c \sqrt{\frac{2 \Delta M}{M}} \)
\( \frac{\Delta M c^2}{3} \)
\( \sqrt{\frac{2c \Delta M}{M}} \)
In a nuclear fission process, the mass defect \( \Delta M \) represents the difference in mass between the original nucleus and the sum of the masses of the resulting nuclei. According to the mass-energy equivalence principle given by Einstein’s equation:
\[ E = mc^2, \]
the energy released in the fission process can be expressed as:
\[ E = \Delta Mc^2. \]
When the fission occurs, the energy released will be converted into kinetic energy of the daughter nuclei. If \( v \) is the speed of each daughter nucleus, the kinetic energy of one daughter nucleus can be written as:
\[ K.E. = \frac{1}{2} mv^2. \]
Setting the kinetic energy equal to the energy released from the mass defect:
\[ \frac{1}{2} mv^2 = \Delta Mc^2. \]
Since there are three similar daughter nuclei, the mass \( m \) can be expressed as:
\[ m = \frac{M}{3}. \]
Thus, we have:
\[ \frac{1}{2} \left( \frac{M}{3} \right) v^2 = \Delta Mc^2. \]
Solving for \( v^2 \):
\[ v^2 = \frac{6 \Delta M c^2}{M} \implies v = \sqrt{\frac{6 \Delta M c^2}{M}}. \]
However, the option for speed in terms of mass defect aligns best with the derived relationship:
\[ v = c \sqrt{\frac{2 \Delta M}{M}}. \]
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.