The problem involves the fission of a heavy nucleus \( N \), which undergoes the reaction:
\( N \rightarrow P + Q \)
Where \( P \) and \( Q \) are two lighter nuclei formed during the fission process. The masses of the nuclei are denoted by \( M_N \), \( M_P \), and \( M_Q \) for \( N \), \( P \), and \( Q \), respectively. The quantity \( \delta \) is defined as:
\( \delta = M_N - M_P - M_Q \)
Here, \( E_P \) and \( E_Q \) are the kinetic energies of the nuclei \( P \) and \( Q \), respectively. The speeds of \( P \) and \( Q \) are given as \( v_P \) and \( v_Q \), and \( c \) is the speed of light.
Step 1: Conservation of Energy
In the fission process, the total energy is conserved. The initial rest mass energy of the nucleus \( N \) is given by \( E_N = M_N c^2 \). After the fission, the total energy is the sum of the rest mass energies and the kinetic energies of the fission products \( P \) and \( Q \):
\( E_{\text{total}} = M_P c^2 + M_Q c^2 + E_P + E_Q \)
Using the principle of conservation of energy:
\( M_N c^2 = M_P c^2 + M_Q c^2 + E_P + E_Q \)
This implies that the sum of the kinetic energies \( E_P + E_Q \) is related to the mass defect \( \delta \) by:
\( E_P + E_Q = \delta c^2 \)
Step 2: Conservation of Momentum
Since the nucleus \( N \) is initially at rest, the total momentum of the system must be zero after the fission. This means that the momenta of \( P \) and \( Q \) must be equal in magnitude and opposite in direction:
\( \vec{p}_P = - \vec{p}_Q \)
The magnitudes of the momenta are given by:
\( p_P = p_Q \)
Step 3: Relating Momentum to Kinetic Energy
The kinetic energy of each particle is related to its momentum by the relativistic equation:
\( E = \sqrt{p^2 c^2 + M^2 c^4} - M c^2 \)
For \( P \), the energy is:
\( E_P = \sqrt{p_P^2 c^2 + M_P^2 c^4} - M_P c^2 \)
Similarly, for \( Q \), the energy is:
\( E_Q = \sqrt{p_Q^2 c^2 + M_Q^2 c^4} - M_Q c^2 \)
Step 4: Result for Momentum
Since \( p_P = p_Q \), the magnitude of the momentum for both particles is the same. By using the conservation of energy and momentum, it can be shown that the magnitude of the momentum for both \( P \) and \( Q \) is given by:
\( p_P = p_Q = c \sqrt{2 \mu \delta} \)
Where \( \mu \) is the reduced mass, defined as:
\( \mu = \frac{M_P M_Q}{M_P + M_Q} \)
Final Answer:
The magnitude of momentum for \( P \) as well as \( Q \) is \( c \sqrt{2 \mu \delta} \), where \( \mu = \frac{M_P M_Q}{M_P + M_Q} \).
Mass Defect and Energy Released in the Fission of \( ^{235}_{92}\text{U} \)
When a neutron collides with \( ^{235}_{92}\text{U} \), the nucleus gives \( ^{140}_{54}\text{Xe} \) and \( ^{94}_{38}\text{Sr} \) as fission products, and two neutrons are ejected. Calculate the mass defect and the energy released (in MeV) in the process.
Given:
Let $ S $ denote the locus of the point of intersection of the pair of lines $$ 4x - 3y = 12\alpha,\quad 4\alpha x + 3\alpha y = 12, $$ where $ \alpha $ varies over the set of non-zero real numbers. Let $ T $ be the tangent to $ S $ passing through the points $ (p, 0) $ and $ (0, q) $, $ q > 0 $, and parallel to the line $ 4x - \frac{3}{\sqrt{2}} y = 0 $.
Then the value of $ pq $ is
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.