Neutrino and axion hot dark matter bounds after WMAP-7

TL;DR

This paper updates cosmological limits on neutrino and axion hot dark matter using WMAP-7, SDSS, and HST data, providing tighter constraints on their masses and contributions to dark matter.

Contribution

It presents the most restrictive cosmological bounds on neutrino and axion masses after analyzing multiple datasets, improving previous limits.

Findings

95% C.L. upper limit on neutrino mass: 0.44 eV

95% C.L. upper limit on axion mass: 0.91 eV

CMB data alone constrains neutrino mass to 1.19 eV

Abstract

We update cosmological hot dark matter constraints on neutrinos and hadronic axions. Our most restrictive limits use 7-year data from the Wilkinson Microwave Anisotropy Probe for the cosmic microwave background anisotropies, the halo power spectrum (HPS) from the 7th data release of the Sloan Digital Sky Survey, and the Hubble constant from Hubble Space Telescope observations. We find 95% C.L. upper limits of \sum m_\nu<0.44 eV (no axions), m_a<0.91 eV (assuming \sum m_\nu=0), and \sum m_\nu<0.41 eV and m_a<0.72 eV for two hot dark matter components after marginalising over the respective other mass. CMB data alone yield \sum m_\nu<1.19 eV (no axions), while for axions the HPS is crucial for deriving m_a constraints. This difference can be traced to the fact that for a given hot dark matter fraction axions are much more massive than neutrinos.