Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
arXiv:2511.13826 · doi:10.1093/mnras/stag927
Abstract
We present Aletheia, a new emulator of the non-linear matter power spectrum, , built upon the evolution mapping framework. This framework addresses the limitations of traditional emulation by focusing on -independent cosmological parameters, which can be separated into those defining the linear power spectrum shape () and those affecting only its amplitude evolution (). The combined impact of evolution parameters and redshift is compressed into a single amplitude parameter, . Aletheia uses a two-stage Gaussian Process emulation: a primary emulator predicts the non-linear boost factor as a function of () and for fixed evolution parameters, while a second one applies a small linear correction based on the integrated growth history. The emulator is trained on shape parameters spanning 5 of Planck constraints and a wide clustering range , providing predictions for . We validate Aletheia against N-body simulations, demonstrating sub-percent accuracy. When tested on a suite of dynamic dark energy models, the full emulator's predictions show a variance of approximately 0.2%, a factor of five smaller than that of the state-of-the-art EuclidEmulator2 (around 1% variance). Furthermore, Aletheia maintains sub-percent accuracy for the best-fit dynamic dark energy cosmology from recent DESI data, a model whose parameters lie outside the training ranges of most conventional emulators. This demonstrates the power of the evolution mapping approach, providing a robust and extensible tool for precision cosmology.
13 pages, 10 figures, submitted to MNRAS. The Aletheia Python package is available on PyPI at https://pypi.org/project/AletheiaCosmo/0.1.0/. Code and documentation are available at https://gitlab.mpcdf.mpg.de/arielsan/aletheia
References in corpus (21)
- The Pantheon+ Analysis: Cosmological Constraints
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- Transients from Initial Conditions in Cosmological Simulations
- Euclid. I. Overview of the Euclid mission
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
- Cosmological parameters derived from the final (PR4) Planck data release
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample
- KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey
- Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions
- COMET: Clustering Observables Modelled by Emulated perturbation Theory
- CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
- Evolution mapping: a new approach to describe matter clustering in the non-linear regime
- Evolution mapping II: describing statistics of the non-linear cosmic velocity field
- Extending evolution mapping to massive neutrinos with COMET
- Extending CSST Emulator to post-DESI era
- Computing Nonlinear Power Spectra Across Dynamical Dark Energy Model Space with Neural ODEs