We construct a second-order, linear, and fully decoupled scheme for Rayleigh–Bénard convection between Navier-slip walls. The nonlinear terms are treated explicitly and multiplied by a scalar with exact value and no energy contributed to the continuous problem. As a result, each BDF2 step, with a rotational pressure correction, solves only constant-coefficient linear problems. For the time discretization, we prove that, for any time-step, the energy decays when the walls have equal temperatures, under a condition on the thermal weight, and the energy is bounded on finite time intervals when heated from below. Relaxing the scalar towards preserves both estimates. Energy stability does not control the accuracy of the scalar; the velocity and temperature fields are computed with its unrelaxed value, whose deviation from scales like for kinetic energy , time-scale of the flow, and weight of the scalar equation. In our tests, choosing comparable to keeps this deviation small and doubles the largest time-step for which steady rolls are reproduced to a relative difference of . With Taylor–Hood elements, we observe second-order convergence in time, recover the critical Rayleigh numbers, and match published Nusselt numbers to within . A three-dimensional implementation passes corresponding validation tests.

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