Ten-dimensional neural network emulator for the nonlinear matter power spectrum
arXiv:2507.07177 · doi:10.1103/8yzy-t59w
Abstract
We present GokuNEmu, a ten-dimensional neural network emulator for the nonlinear matter power spectrum, designed to support next-generation cosmological analyses. Built on the Goku -body simulation suite and the T2N-MusE emulation framework, GokuNEmu predicts the matter power spectrum with average accuracy for redshifts and scales . The emulator models a 10D parameter space that extends beyond CDM to include dynamical dark energy (characterized by and ), massive neutrinos (), the effective number of neutrinos (), and running of the spectral index (). Its broad parameter coverage, particularly for the extensions, makes it the only matter power spectrum emulator capable of testing recent dynamical dark energy constraints from DESI. In addition, it requires only 2 milliseconds to predict a single cosmology on a laptop, orders of magnitude faster than existing emulators. These features make GokuNEmu a uniquely powerful tool for interpreting observational data from upcoming surveys such as LSST, Euclid, the Roman Space Telescope, and CSST.
9 pages, 5 figures, 1 table. Updated to match the version published in Phys. Rev. Lett
References in corpus (42)
- Exploring the Expansion History of the Universe
- Accelerating Universes with Scaling Dark Matter
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- Dark Matter Candidates from Particle Physics and Methods of Detection
- 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
- Massive neutrinos and cosmology
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
- Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- The Physics of Cosmic Acceleration
- The Quijote simulations
- The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum
- Cosmology from the Chinese Space Station Optical Survey (CSS-OS)
- The Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power Spectrum
- The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
- Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
- Cosmological -body simulations with suppressed variance
- Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
- An efficient implementation of massive neutrinos in non-linear structure formation simulations
- Mapping the Cosmological Expansion
- Neutrino mass in cosmology: status and prospects
- The Aemulus Project I: Numerical Simulations for Precision Cosmology
- The Mira-Titan Universe II: Matter Power Spectrum Emulation
- The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
- The Aemulus Project III: Emulation of the Galaxy Correlation Function
- The Aemulus Project II: Emulating the Halo Mass Function
- Direct neutrino-mass measurement based on 259 days of KATRIN data
- An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
- The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
- Precision modelling of the matter power spectrum in a Planck-like Universe
- Multi-Fidelity Emulation for the Matter Power Spectrum using Gaussian Processes
- CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
- A neural network emulator for the Lyman- 1D flux power spectrum
- BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
- Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
- CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
- MF-Box: Multi-fidelity and multi-scale emulation for the matter power spectrum
- Design and optimization of neural networks for multifidelity cosmological emulation