1. Using the Hamiltonian:
The Hamiltonian of the system is given by:
\[ H(p, q) = \frac{p^2}{2m} + q^2 A(q) \]
The Hamiltonian represents the total energy of the system, which is a sum of kinetic and potential energies.
2. Equations of motion:
The equations of motion are given by Hamilton's equations. For position \( q \) and momentum \( p \), we have:
\[ \frac{dq}{dt} = \frac{\partial H}{\partial p} = \frac{p}{m} \]
and
\[ \frac{dp}{dt} = -\frac{\partial H}{\partial q} = -2q A(q) - q^2 \frac{dA(q)}{dq} \]
3. Substitute the equation of motion:
According to the problem, we are given that:
\[ m \frac{d^2 q}{dt^2} = -5q A(q) \]
Using \( \frac{dq}{dt} = \frac{p}{m} \), we get:
\[ m \frac{d^2 q}{dt^2} = \frac{d}{dt} \left( \frac{p}{m} \right) = \frac{dp}{dt} \]
Substituting the expression for \( \frac{dp}{dt} \):
\[ m \frac{d^2 q}{dt^2} = -2q A(q) - q^2 \frac{dA(q)}{dq} \]
Comparing this with the given equation:
\[ -2q A(q) - q^2 \frac{dA(q)}{dq} = -5q A(q) \]
4. Solve for \( \frac{dA(q)}{dq} \):
Simplifying:
\[ -q^2 \frac{dA(q)}{dq} = -3q A(q) \quad \Rightarrow \quad \frac{dA(q)}{dq} = \frac{3A(q)}{q} \]
Comparing with \( \frac{dA(q)}{dq} = n \frac{A(q)}{q} \), we find:
\[ n = \boxed{3} \]
| 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: