canonical setting

Strongly log-concave + log-smooth

πeV\pi\propto e^{-V}, αI2VβI\alpha I\preceq\nabla^2V\preceq\beta I, κ=β/α\kappa=\beta/\alpha.

Upper and lower bounds

Comparison table

6 scoped results. Tildes suppress logarithmic factors.

Edit table
Best-known and comparison results for Strongly log-concave + log-smooth
ResultAlgorithm or modelComplexityGuaranteeOracle / startAssumptions and notesReviewSources
best upperExact ULD / FORSO~(κ2/3d1/3polylog(1/ε))\widetilde O(\kappa^{2/3}d^{1/3}\,\operatorname{polylog}(1/\varepsilon))Rqε2\mathcal R_q\le\varepsilon^2V,VV,\nabla VCold start under the paper's setupExact path-space rejection implementation; fixed Rényi order.Newest claimed frontier; theorem-level transcription still needs human checking.Citedpreprint
best lowerGeneral first-order oracle lower boundΩ~(min{κlogd,d})\widetilde\Omega(\min\{\sqrt\kappa\log d,d\})Constant total-variation accuracyV,VV,\nabla V queriesAny randomized algorithm in the stated modelGaussian subclass; parameter ranges in the theorem.Fixed d2d\ge2 also has the tight Θd(logκ)\Theta_d(\log\kappa) dependence.Checkedpublished
upperMALAO~(κdpolylog(1/ε))\widetilde O(\kappa\sqrt d\,\operatorname{polylog}(1/\varepsilon))μNπTVε\lVert\mu_N-\pi\rVert_{\rm TV}\le\varepsilonV,VV,\nabla Vχ2(μ0π)=O(1)\chi^2(\mu_0\Vert\pi)=O(1)Standard strong convexity and smoothness only.Stable high-accuracy baseline; warm-start cost is separate.Checkedmonograph
upperRandomized-midpoint ULMCO~(κ5/6d1/3/ε2/3)\widetilde O(\kappa^{5/6}d^{1/3}/\varepsilon^{2/3})μNπTVε\lVert\mu_N-\pi\rVert_{\rm TV}\le\varepsilonV\nabla VKnown mode / specified Gaussian startV(0)=0\nabla V(0)=0; low-accuracy regime.Do not compare directly with polylogarithmic high-accuracy rows.Checkedmonograph
upperBlock-Krylov Gaussian samplerO((dκ)log(d/ε2))O((d\wedge\sqrt\kappa)\log(d/\varepsilon^2))KLε\sqrt{\operatorname{KL}}\le\varepsilonGaussian matrix-vector / gradientCentered Gaussian modelGaussian subclass.Nearly tight for Gaussians, not a general-target upper bound.Checkedmonograph
lowerMALA lower boundΩ~(κdlog(1/ε))\widetilde\Omega(\kappa\sqrt d\log(1/\varepsilon))Constant warm start; TV accuracyMALA transitionsχ2(μ0π)1\chi^2(\mu_0\Vert\pi)\lesssim1Algorithm-specific, for every fixed MALA step size.Matches the warm-start MALA upper bound up to logarithms.Checkedmonograph

Scope

The default oracle returns V(x)V(x) and V(x)\nabla V(x). Rows are not directly comparable unless the error metric, initialization, and additional smoothness assumptions match.

Reading the frontier

The newest high-accuracy upper bound uses exact simulation of underdamped Langevin diffusion and is still a preprint. The checked MALA and randomized-midpoint rows are retained as stable baselines. The general first-order lower bound is much smaller than the newest upper bound, so the oracle-complexity gap remains open.

Conventions

O~\widetilde O and Ω~\widetilde\Omega suppress logarithmic factors. A warm start means bounded Rényi or chi-squared divergence as specified in the row.