Gravity enters the BQ-Dirac algebra as a local Lorentz rotor field: the global boost Λ = diag(U−1, U) of the Lorentz models, with its constant rapidity replaced by a rapidity field χ(r, t). Rapidity potentials feed the BQ-Pauli rotor G = eχσ/2, and its Dirac double Qg = diag(G−1, G) = e−χα/2 boosts the Dirac line element by one similarity. As at the Pauli level, the exact image dRg is flat, and the metric comes from its Galilean limit θ with a Lorentzian quadratic. At the Dirac level that quadratic is simply the square θθ = ds²𝟙, and gμν is the anticommutator of the β-matrices θμ, where the exact dRg,μ only give back the flat g⁰μν. Choose the rapidities that feed the rotor.
Units: c = 1 and rs = 2GM/c² = 1, so ψN = √(rs/r). The equatorial plane θ = π/2 is used for the numbers.
Here γr = cosh χr and γφ = cosh χφ; in steps 2–4 v = c tanh χ is the exact boost speed, from step 5 on v = cχ is the river velocity; sθ = sin θ, η = diag(−1, 1, 1, 1). Three line elements: the flat dR, its exact image dRg (flat), and the Galilean θ (curved).
Rapidity fields, coframe and metric as in de Haas (2026), The Gravitational Rapidity Potential, at the BQ-Pauli level; the Dirac rotor Qg, the boosted basis and the metric as the scalar part of the curved β-products as in de Haas (2025), BQ Dirac Gravity, Sec. 4 and eqs. 173, 191–192. Naming: the paper’s dRg of §4.1 (the Galilean, PG line element) is θ here; dRg here is the exact image, the paper’s A̸G of eq. 124. The paper’s /Gμ = QgβμQg−1 = θaμβ̂a (eqs. 193, 226) joins the two parts that the matrices separate: QgβμQg−1 alone only gives η, the coframe θaμ gives gμν. Reported, not changed: eqs. 146–150 give Qgβ0Qg−1 = cosh ψ β0 + sinh ψ βr for Qg = exp(−½ψβ0βr); with the BQ-Weyl matrices of this site that rotor gives the minus sign, and the plus sign belongs to rotor rapidity −ψ (the time-orientation toggle). The metric is not affected.
Every identity is checked exactly, in both time orientations, in bq_dirac_gravity_rotor.py. Part of the BQ algebra at the Dirac level.