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The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the S8 tension

Elbers, Willem; Frenk, Carlos S.; Jenkins, Adrian; Li, Baojiu; Helly, John C.; Kugel, Roi; Schaller, Matthieu; Schaye, Joop; Braspenning, Joey; Kwan, Juliana; McCarthy, Ian G.; Salcido, Jaime; van Daalen, Marcel P.; Vandenbroucke, Bert; Pascoli, Silvia

The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the S8 tension Thumbnail


Authors

Profile image of Willem Elbers

Willem Elbers willem.h.elbers@durham.ac.uk
Postdoctoral Research Associate

Roi Kugel

Matthieu Schaller

Joop Schaye

Joey Braspenning

Juliana Kwan

Ian G. McCarthy

Jaime Salcido

Marcel P. van Daalen

Bert Vandenbroucke



Abstract

Large-scale structure surveys have reported measurements of the density of matter, Ωm, and the amplitude of clustering, σ8, that are in tension with the values inferred from observations of the cosmic microwave background. While this may be a sign of new physics that slows the growth of structure at late times, strong astrophysical feedback processes could also be responsible. In this work, we argue that astrophysical processes are not independent of cosmology and that their coupling naturally leads to stronger baryonic feedback in cosmological models with suppressed structure formation or when combined with a mechanism that removes dark matter from haloes. We illustrate this with two well-motivated extensions of the Standard Model known to suppress structure formation: massive neutrinos and decaying dark matter. Our results, based on the FLAMINGO suite of hydrodynamical simulations, show that the combined effect of baryonic and non-baryonic suppression mechanisms is greater than the sum of its parts, particularly for decaying dark matter. We also show that the dependence of baryonic feedback on cosmology can be modelled as a function of the ratio fb/c2v~ fb/(Ωmσ8)1/4 of the universal baryon fraction, fb, to a velocity-based definition of halo concentration, c2v, giving an accurate fitting formula for the baryonic suppression of the matter power spectrum. Although the combination of baryonic and non-baryonic suppression mechanisms can resolve the tension, the models with neutrinos and decaying dark matter are challenged by constraints on the expansion history.

Citation

Elbers, W., Frenk, C. S., Jenkins, A., Li, B., Helly, J. C., Kugel, R., Schaller, M., Schaye, J., Braspenning, J., Kwan, J., McCarthy, I. G., Salcido, J., van Daalen, M. P., Vandenbroucke, B., & Pascoli, S. (2025). The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the S8 tension. Monthly Notices of the Royal Astronomical Society, 537(2), 2160-2178. https://doi.org/10.1093/mnras/staf093

Journal Article Type Article
Acceptance Date Jan 13, 2025
Online Publication Date Jan 16, 2025
Publication Date 2025-02
Deposit Date Mar 10, 2025
Publicly Available Date Mar 10, 2025
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 537
Issue 2
Pages 2160-2178
DOI https://doi.org/10.1093/mnras/staf093
Public URL https://durham-repository.worktribe.com/output/3705460

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