What is the physical origin of fluorescence, and why does fluorescence emission occur at longer wavelengths than excitation (Stokes shift)?
Fluorescence is a luminescence phenomenon in which an electronically excited molecule in the lowest singlet excited state (S₁) radiatively relaxes back to the singlet electronic ground state (S₀) via spontaneous photon emission. According to the Franck-Condon principle, electronic excitation occurs quasi-instantaneously (≈ 10⁻¹⁵ s) without nuclear motion, promoting the fluorophore into higher vibrational levels of S₁ (or S₂). Rapid non-radiative relaxation (internal conversion and vibrational thermalization, ≈ 10⁻¹² s) rapidly dissipates vibrational excess energy into solvent heat, dropping the molecule into the vibrational ground level of S₁ (Kasha's rule). Radiative transition S₁ → S₀ subsequently occurs with a characteristic lifetime of 1 to 100 ns. Because vibrational energy is dissipated prior to emission and the molecule returns to vibrationally excited levels of S₀, the emitted photon possesses less energy (hν_em < hν_ex) than the absorbed photon, causing the fluorescence spectrum to be systematically bathochromically shifted toward longer wavelengths (Stokes shift). For quinine sulfate, excitation at 350 nm results in intense sky-blue emission peaking at 450 nm (Stokes shift Δλ = 100 nm).