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FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator

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arxiv 2109.04984 v1 pith:LS2X6NNJ submitted 2021-09-10 astro-ph.CO gr-qc

FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator

classification astro-ph.CO gr-qc
keywords emulatorgravityscalesforgepowersimulationsspectrumcosmological
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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abstract

We present a large suite of cosmological simulations, the FORGE (F-of-R Gravity Emulator) simulation suite, which is designed to build accurate emulators for cosmological observables in galaxy clustering, weak gravitational lensing and galaxy clusters, for the $f(R)$ gravity model. The total of 200 simulations explore the cosmological parameter space around the Planck(2018) cosmology with a Latin hypercube, for 50 combinations of $\bar{f}_{R0}$, $\Omega_m$, $\sigma_8$ and $h$ with all other parameters fixed. For each parameter combination, or node, we ran four independent simulations, one pair using $1024^3$ particles in $500 h^{-1} Mpc$ simulation boxes to cover small scales, and another pair using $512^3$ simulation particles in $1500 h^{-1} Mpc$ boxes for larger scales. Each pair of initial conditions are selected such that sample variance on large scales is minimised on average. In this work we present an accurate emulator for the matter power spectrum in $f(R)$ gravity trained on FORGE. We have verified, using the cross-validation technique, that the emulator accuracy is better than $2.5\%$ for the majority of nodes, particularly around the center of the explored parameter space, up to scales of $k = 10 h Mpc^{-1}$. We have also checked the power spectrum emulator against simulations which are not part of our training set and found excellent agreement. Due to its high accuracy on small scales, the FORGE matter power spectrum emulator is well suited for weak lensing analysis and can play a key tool in constraining $f(R)$ gravity using current and future observational data.

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Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Emulating the nonlinear effects of modified gravity on the matter power spectrum for reconstruction

    astro-ph.CO 2026-07 conditional novelty 6.0

    A neural-network emulator predicts the ratio of nonlinear to linear modified-gravity matter power spectra across a 28-dimensional cosmological and MG parameter space, matching MGCAMB+ReACT to roughly 1–2%.

  2. Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity

    astro-ph.CO 2026-03 conditional novelty 6.0

    An emulator trained on modified-gravity simulations enables MCMC forecasts showing that LSST plus CMB lensing constrains the lensing combination Sigma(z)=mu(1+eta)/2 much better than mu or eta alone, especially at z>2.

  3. Modeling nonlinear scales for dynamical dark energy cosmologies with COLA

    astro-ph.CO 2025-10 unverdicted novelty 6.0

    COLA-based hybrid emulator reproduces nonlinear power spectrum boosts in w0wa models to <2% error vs EuclidEmulator2 and produces <0.3σ shifts in LSST-like cosmic shear parameter constraints.

  4. Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity

    astro-ph.CO 2026-03 unverdicted novelty 5.0

    Emulation of binned modified gravity power spectra to <1% accuracy enables MCMC forecasts that constrain μ and η via LSST large-scale structure combined with CMB lensing, with best sensitivity along the lensing combination Σ.

  5. Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes

    astro-ph.CO 2023-06 conditional novelty 4.0

    Forecasts show Euclid combined probes can constrain log f_R0 at the 1% level for fiducial f_R0=5e-6, distinguishing from LCDM at >3 sigma in optimistic settings.