In the case of paramagnetic materials, the population of ions in the energy states is governed by the Boltzmann distribution.
The probability of an ion being in the lowest energy state is given by: \[ P = \frac{1}{1 + e^{\frac{E}{kT}}} \] where \( E \) is the energy difference between the states, \( k \) is Boltzmann's constant, and \( T \) is the temperature. For paramagnetic ions with angular momentum \( J = \frac{1}{2} \), the energy difference \( E \) between the states is proportional to the magnetic field \( B \), i.e., \( E \propto B \). So, the ratio of magnetic fields required for different probabilities of being in the lowest energy state follows the relation: \[ \frac{B_1}{B_2} = \frac{\ln P_2}{\ln P_1} \] For \( P_1 = 0.8 \) and \( P_2 = 0.6 \), we calculate the ratio as: \[ \frac{B_1}{B_2} = \frac{\ln 0.6}{\ln 0.8} = \frac{2 \ln 2}{\ln \left(\frac{3}{2}\right)} \] Thus, the correct answer is \( \frac{2 \ln 2}{\ln \left( \frac{3}{2} \right)} \).
| Column I | Column II |
(1)![]() | (P) Diamagnetic |
(2)![]() | (Q) Paramagnetic |
(3)![]() | (R) Ferromagnetic |
(4)![]() | (S) Antiferromagnetic |
Consider a two-level system with energy states \( +\epsilon \) and \( -\epsilon \). The number of particles at \( +\epsilon \) level is \( N+ \) and the number of particles at \( -\epsilon \) level is \( N- \). The total energy of the system is \( E \) and the total number of particles is \( N = N+ + N- \). In the thermodynamic limit, the inverse of the absolute temperature of the system is:
(Given: \( \ln N! \approx N \ln N - N \))
A two-level quantum system has energy eigenvalues
\( E_1 \) and \( E_2 \). A perturbing potential
\( H' = \lambda \Delta \sigma_x \) is introduced, where
\( \Delta \) is a constant having dimensions of energy,
\( \lambda \) is a small dimensionless parameter, and
\( \sigma_x = \begin{pmatrix} 0 & 1 \\ 1 & 0 \end{pmatrix} \).
The magnitudes of the first and the second order corrections to
\( E_1 \) due to \( H' \), respectively, are: