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Rabi Model

The quantum Rabi model couples one two-level system to one quantized oscillator mode while retaining both rotating and counter-rotating interaction terms.

The model describes a minimal closed light-matter system: a two-level atom, artificial atom, spin, or qubit interacting with a single cavity or oscillator mode. It is the natural parent model of Jaynes–Cummings when the rotating-wave approximation is not made.

The Hilbert space is a tensor product

H=C2⊗FB,\mathcal H = \mathbb C^2 \otimes \mathcal F_B,

where FB\mathcal F_B is the Fock space of one bosonic oscillator mode.

A common convention is

H=ℏωca†a+ℏω02σz+ℏg(a+a†)σx.H = \hbar\omega_c a^\dagger a + \frac{\hbar\omega_0}{2}\sigma_z + \hbar g \left(a+a^\dagger\right)\sigma_x.

Equivalently, since σx=σ++σ−\sigma_x=\sigma_++\sigma_-, the interaction contains

aσ++a†σ−+aσ−+a†σ+.a\sigma_+ + a^\dagger\sigma_- + a\sigma_- + a^\dagger\sigma_+.

The last two terms are counter-rotating terms. They are the terms removed in the Jaynes–Cummings rotating-wave approximation.

SymbolMeaning
ωc\omega_coscillator or cavity-mode frequency
ω0\omega_0two-level transition frequency
gglight-matter coupling strength
a,a†a,a^\daggerbosonic annihilation and creation operators
σα\sigma_\alphaPauli operators on the two-level system

The quantum Rabi model has a conserved parity symmetry, but it does not conserve excitation number. It is exactly solvable in a specialized analytic sense and is also widely treated numerically by truncating the oscillator basis with convergence checks.

When gg is weak and the system is near resonance, the rotating-wave approximation reduces the model to Jaynes–Cummings.

  • Dressed eigenenergies.
  • Photon-number distribution.
  • Two-level inversion.
  • Parity sectors.
  • Bloch-Siegert shift from counter-rotating terms.

The Rabi model teaches the difference between semiclassical Rabi oscillations, quantum oscillator coupling, and rotating-wave effective models. It is especially important in strong and ultrastrong coupling regimes where counter-rotating terms are not negligible.

  • Using Jaynes–Cummings formulas after leaving the rotating-wave regime.
  • Assuming excitation number is conserved in the full Rabi model.
  • Confusing classical driven Rabi oscillations with the quantized Rabi model.
  • Interpreting oscillator-basis truncation results without convergence checks.

Which terms in the Rabi interaction fail to conserve the Jaynes–Cummings excitation number?

Solution

The counter-rotating terms aσ−a\sigma_- and a†σ+a^\dagger\sigma_+ change the oscillator and two-level excitation in the same direction, so they change the total excitation number by two units.

  • I. I. Rabi, “On the process of space quantization,” Physical Review 49, 324-328, 1936.
  • I. I. Rabi, “Space quantization in a gyrating magnetic field,” Physical Review 51, 652-654, 1937.
  • D. Braak, “Integrability of the Rabi model,” Physical Review Letters 107, 100401, 2011.