Optimizing the Recovery of Fisher Information in the Dark Matter Power Spectrum
Joachim Harnois-Deraps, Hao-Ran Yu, Tong-Jie Zhang, Ue-Li Pen

TL;DR
This paper demonstrates that combining wavelet filtering and density reconstruction techniques significantly enhances the recovery of Fisher information in dark matter density fields, especially at small scales, with implications for cosmological parameter estimation.
Contribution
The study introduces a combined approach using Wavelet Non-Linear Wiener Filter and density reconstruction to improve Fisher information recovery in dark matter simulations, showing synergistic effects.
Findings
Fisher information plateau increases by over an order of magnitude at k > 1.0h/Mpc for particles.
Combined techniques outperform individual methods, with a recovery boost of 3-5 times.
Reconstruction has limited effect on halo catalogues, but wavelet filtering significantly boosts information.
Abstract
We combine two Gaussianization techniques - Wavelet Non-Linear Wiener Filter (WNLWF) and density reconstruction - to quantify the recovery of Fisher information that is lost in the gravitational collapse. We compute a displacement fields, in analogy with the Zel'dovich approximation, and apply a Wavelet Non-Linear Wiener Filter that decomposes the reconstructed density fields into a Gaussian and a non-Gaussian component. From a series of 200 realizations of N-body simulations, we compute the recovery performance for density fields obtained with both dark matter particles and haloes. We find that the height of the Fisher information trans-linear plateau is increased by more than an order of magnitude at k > 1.0h/Mpc for particles, whereas either technique alone offers an individual recovery boost of only a factor of three to five. We conclude that these two techniques work in a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
