Euclid preparation: II. the EUCLIDEMULATOR - a tool to compute the cosmology dependence of the nonlinear matter power spectrum


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Date

2019-04

Publication Type

Journal Article

ETH Bibliography

yes

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Abstract

We present a new power spectrum emulator named EuclidEmulator that estimates the nonlinear correction to the linear dark matter power spectrum depending on the six cosmological parameters ωb, ωₘ, nₛ, h, w₀, and σ₈. It is constructed using the uncertainty quantification software UQLab using a spectral decomposition method called polynomial chaos expansion. All steps in its construction have been tested and optimized: the large high-resolution N-body simulations carried out with PKDGRAV3 were validated using a simulation from the Euclid Flagship campaign and demonstrated to have converged up to wavenumbers k≈5hMpc−¹ for redshifts z ≤ 5. The emulator is based on 100 input cosmologies simulated in boxes of (1250 Mpc/h)³ using 2048³ particles. We show that by creating mock emulators it is possible to successfully predict and optimize the performance of the final emulator prior to performing any N-body simulations. The absolute accuracy of the final nonlinear power spectrum is as good as one obtained with N-body simulations, conservatively, ∼1 per cent for k≲1hMpc−¹ and z ≲ 1. This enables efficient forward modelling in the nonlinear regime, allowing for estimation of cosmological parameters using Markov Chain Monte Carlo methods. EuclidEmulator has been compared to HALOFIT, CosmicEmu, and NGenHalofit, and shown to be more accurate than these other approaches. This work paves a new way for optimal construction of future emulators that also consider other cosmological observables, use higher resolution input simulations, and investigate higher dimensional cosmological parameter spaces.

Publication status

published

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Book title

Volume

484 (4)

Pages / Article No.

5509 - 5529

Publisher

Oxford University Press

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Edition / version

Methods

Software

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Subject

methods: numerical; methods: statistical; cosmological parameters; Large-scale structure of Universe

Organisational unit

03962 - Sudret, Bruno / Sudret, Bruno check_circle
03928 - Refregier, Alexandre / Refregier, Alexandre check_circle

Notes

It was possible to publish this article open access thanks to a Swiss National Licence with the publisher.

Funding

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