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Pauli Hamiltonian

This is a compact Hamiltonian card. The low-energy equation, magnetic-factor convention, Zeeman and Landau structure, and validity regime are owned by the Pauli Equation; the g=2g=2 reduction is derived on Dirac to Pauli.

For charge qq and

π=p^−qA,\boldsymbol\pi = \hat{\mathbf p}-q\mathbf A,

the Pauli Hamiltonian with g=2g=2 is

H=π22m+qΦ−qℏ2mσ⋅B.H = \frac{\boldsymbol\pi^2}{2m} + q\Phi - \frac{q\hbar}{2m} \boldsymbol\sigma\cdot\mathbf B.

Equivalently,

H=12m(σ⋅π)2+qΦ.H = \frac{1}{2m} \left( \boldsymbol\sigma\cdot\boldsymbol\pi \right)^2 + q\Phi.

The free Pauli operator acts on HP=L2(R3,C2)\mathcal H_P=L^2(\mathbb R^3,\mathbb C^2) with dense domain H2(R3,C2)H^2(\mathbb R^3,\mathbb C^2) and codomain HP\mathcal H_P. For prescribed backgrounds, the self-adjoint realization is determined by the regularity and growth of A\mathbf A, Φ\Phi, and B\mathbf B; a magnetic Sobolev domain is the natural replacement when the covariant derivatives are unbounded. The formula alone does not determine that domain.

On a bounded region, Dirichlet, magnetic Neumann, or another stated self-adjoint boundary condition is part of the Hamiltonian and affects its spectrum. Gauge-related potentials must be compared with the corresponding unitary phase transformation and consistently transformed boundary data.

The common positive-energy phase e−imc2t/ℏe^{-imc^2t/\hbar} has been removed, so the displayed Pauli energy zero is shifted downward by mc2mc^2 relative to the positive-energy Dirac branch. If the backgrounds depend on time, a unitary propagator additionally requires suitable time regularity and compatible domains for H(t)H(t).

  • Nonrelativistic two-component spinor in the operator setting stated above.
  • External electromagnetic potentials are prescribed.
  • The displayed magnetic coupling uses g=2g=2 and omits anomalous magnetic moment terms.
  • The sign of qq is explicit.
  • The identity (σ⋅π)2=π2−qℏσ⋅B(\boldsymbol\sigma\cdot\boldsymbol\pi)^2=\boldsymbol\pi^2-q\hbar\boldsymbol\sigma\cdot\mathbf B reproduces the displayed Zeeman term.
  • Setting Φ=A=B=0\Phi=\mathbf A=\mathbf B=0 gives the spin-degenerate free Hamiltonian p^2/(2m)\hat{\mathbf p}^{2}/(2m).
  • Every term has dimensions of energy, and the signed-qq electron term has the correct Zeeman sign.
  • Gauge-related potentials give unitarily equivalent dynamics when the spinor and boundary data are transformed consistently.
  • Losing the sign of the Zeeman term for electrons.
  • Forgetting that πi\pi_i components fail to commute in a magnetic field.
  • Treating the Pauli Hamiltonian as fully relativistic.
  • Omitting spinor structure and using a scalar wavefunction.
  • W. Pauli, “Zur Quantenmechanik des magnetischen Elektrons”, Zeitschrift für Physik 43, 601-623, 1927.
  • J. J. Sakurai, Advanced Quantum Mechanics, Addison-Wesley, 1967.