Rate of transitions between quantum states due to a perturbation
Speed of light in a vacuum
Strength of the strong nuclear force
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The Correct Option isB
Solution and Explanation
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.