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Future CMB tests of dark matter: Ultralight axions and massive neutrinos

Hlozek, Renée, Marsh, David J. E., Grin, Daniel, Allison, Rupert, Dunkley, Jo and Calabrese, Erminia 2017. Future CMB tests of dark matter: Ultralight axions and massive neutrinos. Physical Review D 95 (12) , 123511. 10.1103/PhysRevD.95.123511

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Abstract

Measurements of cosmic microwave background (CMB) anisotropies provide strong evidence for the existence of dark matter and dark energy. They can also test its composition, probing the energy density and particle mass of different dark-matter and dark-energy components. CMB data have already shown that ultralight axions (ULAs) with mass in the range 10 − 32     eV → 10 − 26     eV compose a fraction ≲ 0.01 of the cosmological critical density. The next Stage-IV CMB experiment (CMB-S4) (assuming a 1 arcmin beam and ∼ 1     μ K − arcmin noise levels over a sky fraction of 0.4) to the density of ULAs and other dark-sector components is assessed. CMB-S4 data should be ∼ 10 times more sensitive to the ULA energy density than Planck data alone, across a wide range of ULA masses 10 − 32 ≲ m a ≲ 10 − 23     eV , and will probe axion decay constants of f a ≈ 1 0 16     GeV , at the grand unified scale. CMB-S4 could improve the CMB lower bound on the ULA mass from ∼ 10 − 25     eV to 10 − 23     eV , nearing the mass range probed by dwarf galaxy abundances and dark-matter halo density profiles. These improvements will allow for a multi- σ detection of percent-level departures from CDM over a wide range of masses. Much of this improvement is driven by the effects of weak gravitational lensing on the CMB, which breaks degeneracies between ULAs and neutrinos. We also find that the addition of ULA parameters does not significantly degrade the sensitivity of the CMB to neutrino masses. These results were obtained using the axionCAMB code (a modification to the CAMB Boltzmann code), presented here for public use.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Subjects: Q Science > QC Physics
Publisher: American Physical Society
ISSN: 2470-0010
Date of First Compliant Deposit: 12 June 2017
Date of Acceptance: 1 May 2017
Last Modified: 13 Jun 2017 08:42
URI: http://orca-mwe.cf.ac.uk/id/eprint/101382

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