Hydrogen Atom: Model and Hamiltonian
Hydrogen is the electron–proton Coulomb problem after separating center-of-mass motion. This reference identifies the ideal nonrelativistic model, its Hamiltonian, and its limits. The Hydrogen Atom teaching page derives the bound-state solution; Hydrogen Spectrum: Formula Reference and Hydrogen Radial Wavefunctions: Formula Reference supply calculation formulas.
Coulomb model and Hamiltonian
Section titled “Coulomb model and Hamiltonian”For one electron and a point nucleus of charge and mass , define the relative coordinate and reduced mass
In SI units, with , the internal Hamiltonian is
Ordinary hydrogen has and . The total Hamiltonian also contains free center-of-mass kinetic energy ; quoted atomic levels are internal energies. Replacing by is the infinite-nuclear-mass approximation.
| Model feature | Definition or exact target |
|---|---|
| Degrees of freedom | Electron–nucleus relative coordinate; spin omitted |
| Hilbert space | |
| Bound-state labels | ; ; |
| Bound energies | |
| Spatial shell degeneracy | ; only when spin is appended without spin-dependent interactions |
| Energy zero | Separated electron and nucleus; continuum threshold |
| Parity | |
| Exact solvability | Bound eigenfunctions and energies; analytic Coulomb continuum functions and phases |
| Extra symmetry | Conserved Runge–Lenz structure explains the additional Coulomb degeneracy |
Here . The Coulomb operator has its standard self-adjoint realization: bound states are square integrable, regular at the origin, and decay at infinity. In the radial representation , the regular boundary condition is . Radial Wavefunctions distinguishes , , and radial probability.
In Hartree atomic units with an infinitely heavy nucleus,
The mass approximation is part of this compact form. Translate Coulomb and unit conventions before combining SI, Gaussian, natural-unit, or atomic-unit formulas.
Physical scope and corrections
Section titled “Physical scope and corrections”Exact solvability applies to instantaneous point-Coulomb interaction without relativity, spin interactions, nuclear structure, radiation coupling, or external fields. It does not make matrix elements, continuum normalization, or precision corrections trivial. Low-lying states require for a controlled nonrelativistic description.
| Additional physics | Consequence and explanation |
|---|---|
| Relativistic kinematics and spin–orbit terms | Fine structure; binding is of order , fine structure of order |
| Radiative corrections | Lamb shifts and other level shifts |
| Nuclear spin and magnetic moment | Hyperfine structure |
| Finite nuclear charge radius | Short-distance shifts, especially for states sampling the origin; see hydrogen as an atomic prototype |
| External electric or magnetic fields | Stark and Zeeman shifts and state mixing |
| Coupling to radiation | Transition rates, linewidths, and finite excited-state lifetimes |
| Additional electrons | Screening, exchange, correlation, and antisymmetry; independent exact hydrogen orbitals no longer solve the problem |
Excited eigenstates of the static Coulomb Hamiltonian have infinite lifetime. Spontaneous emission requires coupling to electromagnetic modes. Orbitals describe wavefunctions, not electron trajectories; their nodes and choice of real or complex basis are explained in Atomic Orbitals.
Related Coulomb systems
Section titled “Related Coulomb systems”| System | Change and limitation |
|---|---|
| Hydrogenic ions | ; relativistic and finite-size effects grow with |
| Deuterium and tritium | Nuclear mass and structure change; reduced mass is only the leading isotope correction |
| Positronium | Equal electron and positron masses; annihilation, spin, and QED effects matter |
| Muonic atoms | Heavier orbiting particle and smaller radius increase sensitivity to nuclear structure |
| Coulomb scattering | Positive-energy sector requires continuum and long-range scattering conventions |
| Alkali valence electrons | Core screening and quantum defects replace exact Coulomb degeneracy |
| Helium and many-electron atoms | Electron–electron interaction prevents exact independent hydrogen solutions |
Neutral helium is not hydrogenic; the one-electron ion is.
Observables and numerical checks
Section titled “Observables and numerical checks”The characteristic length is . These targets make hydrogen useful for checking radial solvers and basis calculations.
| Check | Exact point-Coulomb target |
|---|---|
| Bound energies and spatial degeneracy | and |
| Ground radial probability maximum | |
| Ground radial moments | , |
| Virial relation | |
| Angular eigenvalues | and |
| Radial boundary conditions | and square-integrable decay |
A numerical check must also state the origin treatment, outer boundary, angular sector, energy zero, grid or basis, and convergence with resolution and box size. Radial Schrödinger Solvers gives that workflow.
Electric-dipole observables probe transition amplitudes, with and polarization-dependent in the ideal basis; Dipole Transitions gives the tensor-operator statement. Angular momentum and spin determine magnetic response once the relevant terms are included. Ionization requires continuum flux rather than bound-state normalization.
References
Section titled “References”- H. A. Bethe and E. E. Salpeter, Quantum Mechanics of One- and Two-Electron Atoms, Springer, 1957.
- C. Cohen-Tannoudji, B. Diu, and F. Laloë, Quantum Mechanics, 2 vols., Wiley, 1977.
- D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
- L. D. Landau and E. M. Lifshitz, Quantum Mechanics: Non-Relativistic Theory, 3rd ed., Pergamon, 1977.
- R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.