An Introduction to Modern Astrophysics · Problem 5.15

Telescopes — Carroll & Ostlie

Physics — Astrophysics · heisenberg-uncertainty-spectral-broadening

Problem

An electron spends roughly 10−810^{-8} s in the first excited state of the hydrogen atom before making a spontaneous downward transition to the ground state. (a) Use Heisenberg's uncertainty principle, Eq. (5.20), to determine the uncertainty ΔE\Delta E in the energy of the first excited state. (b) Calculate the uncertainty Δλ\Delta\lambda in the wavelength of the photon involved in a transition (either upward or downward) between the ground and first excited states of the hydrogen atom. Why can you assume that ΔE=0\Delta E = 0 for the ground state? This increase in the width of a spectral line is called natural broadening.

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