Control variates from Eulerian and Lagrangian perturbation theory: Application to the bispectrum

Control variates have seen recent interest as a powerful technique to reduce the variance of summary statistics measured from costly cosmological \(N\)-body simulations. Of particular interest are the class of control variates which are analytically calculable, such as the recently introduced ‘Zeldovich control variates’ for the power spectrum of matter and biased tracers. In this work we present the construction of perturbative control variates in Eulerian and Lagrangian perturbation theory, and adopt the matter bispectrum as a case study. Eulerian control variates are analytically tractable for all \(n\)-point functions, but we show that their correlation with the \(N\)-body \(n\)-point function decays at a rate proportional to the sum-of-squared wavenumbers, hampering their utility. We show that the Zeldovich approximation, while possessing an analytically calculable bispectrum, is less correlated at low-\(k\) than its Eulerian counterpart. We introduce an alternative – the ‘shifted control variate’ – which can be constructed to have the correct tree-level \(n\)-point function, is Zeldovich-resummed, and in principle has an analytically tractable bispectrum. We find that applying this shifted control variate to the \(z=0.5\) matter bispectrum is equivalent to averaging over \(10^4\) simulations for the lowest-\(k\) triangles considered. With a single \(V=1({\rm Gpc}/h)^3\) \(N\)-body simulation, for a binning scheme with \(N\approx 1400\) triangles from \(k_{\rm min} = 0.04 h {\rm Mpc}^{-1}\) to \(k_{\rm \max} = 0.47 h {\rm Mpc}^{-1}\), we obtain sub-2% precision for every triangle configuration measured. This work enables the development of accurate bispectrum emulators – a probe of cosmology well-suited to simulation-based modeling – and lays the theoretical groundwork to extend control variates for the entire \(n\)-point hierarchy.