On the road to per cent accuracy – III. Non-linear reaction of the matter power spectrum to massive neutrinos

Cataneo, M.; Emberson, J. D.; Inman, D.; Harnois-Déraps, J.; Heymans, C.

doi:10.1093/mnras/stz3189

Title: On the road to per cent accuracy – III. Non-linear reaction of the matter power spectrum to massive neutrinos

Journal Article · Fri Nov 15 00:00:00 EST 2019 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stz3189· OSTI ID:1714387

Cataneo, M. ^[1]; Emberson, J. D. ^[2];

^[3];

^[1]; Heymans, C. ^[4]

Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
CPS Division, Argonne National Laboratory, Lemont, IL 60439, USA
Center for Cosmology and Particle Physics, Department of Physics, New York University, 726 Broadway, New York, NY 10003, USA
Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK, German Centre for Cosmological Lensing (GCCL), Astronomisches Institut, Ruhr-Universität Bochum, Universitätsstr 150, D-44801 Bochum, Germany

ABSTRACT We analytically model the non-linear effects induced by massive neutrinos on the total matter power spectrum using the halo model reaction framework of Cataneo et al. In this approach, the halo model is used to determine the relative change to the matter power spectrum caused by new physics beyond the concordance cosmology. Using standard fitting functions for the halo abundance and the halo mass–concentration relation, the total matter power spectrum in the presence of massive neutrinos is predicted to per cent-level accuracy, out to $$k=10 \,{ h}\,{\rm Mpc}^{-1}$$. We find that refining the prescriptions for the halo properties using N-body simulations improves the recovered accuracy to better than 1 per cent. This paper serves as another demonstration for how the halo model reaction framework, in combination with a single suite of standard Λ cold dark matter (ΛCDM) simulations, can recover per cent-level accurate predictions for beyond ΛCDM matter power spectra, well into the non-linear regime.

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Research Organization:: Argonne National Laboratory (ANL), Argonne, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC); European Research Council (ERC)

Contributing Organization:: Fritz Haber Institute of the Max Planck Society (Fritz-Haber-Institut der Max-Planck-Gesellschaft)

Grant/Contract Number:: AC02-06CH11357

OSTI ID:: 1714387

Alternate ID(s):: OSTI ID: 1632118

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Vol. 491 Journal Issue: 3; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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Cited by: 14 works

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