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New MGCAMB tests of gravity with CosmoMC and Cobaya

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arxiv 2305.05667 v2 pith:5W5HAK5S submitted 2023-05-09 astro-ph.CO astro-ph.IMgr-qc

classification astro-ph.COastro-ph.IMgr-qc
keywords darkmgcamboptionversioncambcobayacosmomcenergy
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We present a new version of MGCAMB, a patch for the Einstein-Boltzmann solver CAMB for cosmological tests of gravity. New features include a new cubic-spline parameterization allowing for a simultaneous reconstruction of $\mu$, $\Sigma$ and the dark energy density fraction $\Omega_X$ as functions of redshift, the option to work with a direct implementation of $\mu$, $\Sigma$ (instead of converting to $\mu$, $\gamma$ first), along with the option to test models with a scalar field coupled only to dark matter, and the option to include dark energy perturbations when working with $w\ne -1$ backgrounds, to restore consistency with CAMB in the GR limit. This version of MGCAMB comes with a Python wrapper to run it directly from the Python interface, an implementation in the latest version of CosmoMC, and can be used with Cobaya.

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Cited by 4 Pith papers

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

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

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    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. Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background

    astro-ph.CO 2026-05 unverdicted novelty 5.0 of 10

    Using Planck, DESI, supernovae, and redshift-space distortions, the authors infer that modified gravity, if present, must act only below ~30 Mpc and cannot modify the large scales previously considered.

  3. Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure

    astro-ph.CO 2025-12 conditional novelty 5.0 of 10

    Forecasts indicate that LSS-GW cross-correlations with Stage-IV surveys and Einstein Telescope tighten constraints on modified gravity parameters beyond those from LSS observations alone.

  4. Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys

    astro-ph.CO 2026-02 conditional novelty 4.0 of 10

    Fisher forecasts show BINGO and SKA1-MID 21-cm intensity mapping, combined with Planck priors, could constrain the f(R) gravity parameter B0 down to ~10⁻⁶–10⁻⁸.

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