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Hydrogen Atom Hamiltonian

For a hydrogenic ion with nuclear charge +Ze+Ze and reduced mass μ\mu,

H=p^ 22μ−Ze24πϵ0r.H = \frac{\hat{\mathbf p}^{\,2}}{2\mu} - \frac{Ze^2}{4\pi\epsilon_0 r}.

The ideal nonrelativistic bound-state energies are

En=−μZ2e42(4πϵ0)2ℏ21n2,n=1,2,…E_n = - \frac{\mu Z^2e^4} {2(4\pi\epsilon_0)^2\hbar^2} \frac{1}{n^2}, \qquad n=1,2,\ldots
  • Nonrelativistic two-body Coulomb problem reduced to relative motion.
  • Spin, fine structure, Lamb shift, hyperfine structure, finite nuclear size, and external fields are omitted.
  • The nucleus is represented only through charge and reduced mass.
  • SI units are displayed; atomic or natural units change the appearance.
  • Using electron mass instead of reduced mass when precision matters.
  • Treating the n2n^2 degeneracy as generic for all central potentials.
  • Forgetting which corrections have been omitted.
  • Mixing Gaussian, SI, and atomic-unit Coulomb conventions.
  • H. A. Bethe and E. E. Salpeter, Quantum Mechanics of One- and Two-Electron Atoms, Springer, 1957.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.