Fermi's Golden Rule is a key result in time-dependent perturbation theory within quantum mechanics. It provides a method to calculate the transition rate from an initial quantum state \( |i\rangle \) to a final state \( |f\rangle \) due to a weak perturbation. The rule is expressed as: \[ \Gamma_{i \to f} = \frac{2\pi}{\hbar} |\langle f | H' | i \rangle|^2 \rho(E_f) \] Here:
- \( H' \) is the perturbing Hamiltonian.
- \( \langle f | H' | i \rangle \) is the matrix element representing the coupling between states.
- \( \rho(E_f) \) is the density of final states at energy \( E_f \).
This formula is widely used in quantum optics, nuclear physics, and solid-state physics to estimate how quickly transitions occur when a system is subjected to an external influence like electromagnetic radiation.
Why other options are incorrect: - (A) While decay can involve transitions, Fermi’s Golden Rule specifically addresses induced transitions due to perturbations, not spontaneous decay.
- (C) The speed of light in a vacuum is a fundamental constant, unrelated to perturbation theory.
- (D) The strength of the strong nuclear force is described by quantum chromodynamics, not by Fermi’s rule.