TL;DR
This paper introduces improved initial conditions for cosmological N-body simulations that respect particle linear theory modes and include rescaling, significantly enhancing the accuracy of late-time power spectra and halo statistics.
Contribution
The authors develop initial conditions that incorporate particle linear theory modes and rescaling, improving simulation accuracy and efficiency compared to previous methods.
Findings
Achieved 1% accuracy in power spectrum down to Nyquist frequency
Enhanced halo mass function and clustering accuracy
Demonstrated effectiveness of 2LPT and rescaling in simulations
Abstract
In cosmological -body simulations, the representation of dark matter as discrete "macroparticles" suppresses the growth of structure, such that simulations no longer reproduce linear theory on small scales near . Marcos et al. demonstrate that this is due to sparse sampling of modes near and that the often-assumed continuum growing modes are not proper growing modes of the particle system. We develop initial conditions that respect the particle linear theory growing modes and then rescale the mode amplitudes to account for growth suppression. These ICs also allow us to take advantage of our very accurate -body code Abacus to implement 2LPT in configuration space. The combination of 2LPT and rescaling improves the accuracy of the late-time power spectra, halo mass functions, and halo clustering. In particular, we achieve 1% accuracy in the power…
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