Step 1: The relativistic Hamiltonian for a particle is given by: \[ H = \sqrt{m^2 c^4 + p^2 c^2} + V(x). \] This represents the total energy, where \( m \) is the rest mass and \( p \) is the momentum of the particle.
Step 2: The velocity \( v \) of the particle is related to the momentum \( p \) by the relativistic relation: \[ v = \frac{pc}{\sqrt{p^2 + m^2 c^2}}. \] This expression gives the speed in terms of the relativistic momentum and mass.
Step 3: The Lagrangian \( L \) is derived from the Hamiltonian. The relativistic Lagrangian is given by: \[ L = -m c^2 \sqrt{1 - \frac{v^2}{c^2}} - V(x), \] which accounts for both the kinetic energy and the potential energy.
| 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: