paper

The e-MANTIS emulator: fast and accurate predictions of the halo mass function in CDM and CDM cosmologies

arXiv:2410.05226 · doi:10.1051/0004-6361/202450193

Abstract

In this work, we present a novel emulator of the halo mass function, which we implement in the framework of the e-mantis emulator of gravity models. We also extend e-mantis to cover a larger cosmological parameter space and to include models of dark energy with a constant equation of state CDM. We use a Latin hypercube sampling of the CDM and CDM cosmological parameter spaces, over a wide range, and realize a large suite of more than -body simulations of different volume, mass resolution and random phase of the initial conditions. For each simulation in the suite, we generate halo catalogues using the friends-of-friends halo finder, as well as the spherical overdensity algorithm for different overdensity thresholds. We decompose the corresponding halo mass functions on a B-spline basis, and use this decomposition to train an emulator based on Gaussian processes. The resulting emulator is able to predict the halo mass function for redshifts and for halo masses . The typical HMF errors for SO haloes with at in CDM (respectively CDM) are of order of () up to a transition mass (). For larger masses, the errors are dominated by shot-noise and scale as with () up to . Independently of this general trend, the emulator is able to provide an estimation of its own error as a function of the cosmological parameters, halo mass, and redshift. The e-mantis emulator, which is publicly available, can be used to obtain fast and accurate predictions of the halo mass function in the CDM and CDM non-standard cosmological models.

22 pages, 16 figures. Accepted for publication in A&A. Emulator code available at https://doi.org/10.5281/zenodo.8384121