Facial reconstruction

Search LJMU Research Online

Browse Repository | Browse E-Theses

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

Upadhye, A, Kwan, J, McCarthy, IG, Salcido, J, Helly, JC, Kugel, R, Schaller, M, Schaye, J, Braspenning, J, Elbers, W, Frenk, CS, Van Daalen, MP, Vandenbroucke, B and Broxterman, JC (2024) Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations. Monthly Notices of the Royal Astronomical Society, 529 (2). pp. 1862-1876. ISSN 0035-8711

[img]
Preview
Text
Non-linear CMB lensing with neutrinos and baryons FLAMINGO simulations versus fast approximations.pdf - Published Version
Available under License Creative Commons Attribution.

Download (5MB) | Preview

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 power spectrum emulation using cosmological simulations 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 () up to multipoles L = 3000 (L = 5000) for a νΛCDM 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. 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 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.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences; Astronomy & Astrophysics
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Oxford University Press (OUP)
SWORD Depositor: A Symplectic
Date Deposited: 25 Sep 2024 14:22
Last Modified: 25 Sep 2024 14:30
DOI or ID number: 10.1093/mnras/stae663
URI: https://researchonline.ljmu.ac.uk/id/eprint/24269
View Item View Item