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Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations

Upadhye, Amol; Kwan, Juliana; McCarthy, Ian G; Salcido, Jaime; Helly, John C; Kugel, Roi; Schaller, Matthieu; Schaye, Joop; Braspenning, Joey; Elbers, Willem; Frenk, Carlos S; van Daalen, Marcel P; Vandenbroucke, Bert; Broxterman, Jeger C

Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations Thumbnail


Authors

Amol Upadhye

Juliana Kwan

Ian G McCarthy

Jaime Salcido

Roi Kugel

Joop Schaye

Joey Braspenning

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

Marcel P van Daalen

Bert Vandenbroucke

Jeger C Broxterman



Abstract

Weak lensing of the cosmic microwave background is rapidly emerging as a powerful probe of neutrinos, dark energy, and new
physics. We present a fast computation of the non-linear CMB lensing power spectrum that combines non-linear perturbation
theory at early times with powerspectrum emulation using cosmologicalsimulations at late times.Comparing our calculation with
light-cones from the FLAMINGO 5.6 Gpc cube dark-matter-only simulation, we confirm its accuracy to 1 per cent (2 per cent)
up to multipoles L = 3000 (L = 5000) for a νCDM cosmology consistent with current data. Clustering suppression due to
small-scale baryonic phenomena such as feedback from active galactic nuclei can reduce the lensing power by ∼ 10 per cent.
To our perturbation theory and emulator-based calculation, we add SP(k), a new fitting function for this suppression, and
confirm its accuracy compared to the FLAMINGO hydrodynamic simulations to 4 per cent at L = 5000, with similar accuracy for
massive neutrino models. We further demonstrate that scale-dependent suppression due to neutrinos and baryons approximately
factorize, implying that a careful treatment of baryonic feedback can limit biasing neutrino mass constraints.

Citation

Upadhye, A., Kwan, J., McCarthy, I. G., Salcido, J., Helly, J. C., Kugel, R., …Broxterman, J. C. (2024). Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations. Monthly Notices of the Royal Astronomical Society, 529(2), 1862-1876. https://doi.org/10.1093/mnras/stae663

Journal Article Type Article
Acceptance Date Mar 2, 2024
Online Publication Date Mar 7, 2024
Publication Date 2024-04
Deposit Date May 22, 2024
Publicly Available Date May 22, 2024
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 529
Issue 2
Pages 1862-1876
DOI https://doi.org/10.1093/mnras/stae663
Public URL https://durham-repository.worktribe.com/output/2455753

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
© 2024 The Author(s).
Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.





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