Year: 2009
Type: article
Abstract: We revisit Lyman-α bounds on the dark matter mass in Λ Warm Dark Matter (ΛWDM) models, and derive new bounds in the case of mixed Cold plus Warm models (ΛCWDM), using a set up which is a good approximation for several theoretically well-motivated dark matter models. We combine WMAP5 results with two different Lyman-α data sets, including observations from the Sloan Digital Sky Survey. We pay a special attention to systematics, test various possible sources of error, and compare the results of different statistical approaches. Expressed in terms of the mass of a non-resonantly produced sterile neutrino, our bounds read m NRP ⩾ 8 keV (frequentist 99.7% confidence limit) or m NRP ⩾ 12.1 keV (Bayesian 95% credible interval) in the pure ΛWDM limit. For the mixed model, we obtain limits on the mass as a function of the warm dark matter fraction F WDM . Within the mass range studied here (5 keV < m NRP < ∞ ), we find that any mass value is allowed when F WDM < 0.6 (frequentist 99.7% confidence limit); similarly, the Bayesian joint probability on ( F WDM , 1/ m NRP ) allows any value of the mass at the 95% confidence level, provided that F WDM < 0.35.
Institutions: ETH Zurich, Bogolyubov Institute for Theoretical Physics, Institute for Theoretical Physics, Centre National de la Recherche Scientifique, Laboratoire d'Annecy de Physique Théorique, École Polytechnique Fédérale de Lausanne, European Organization for Nuclear Research, Istituto Nazionale di Fisica Nucleare, Trieste Astronomical Observatory, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
Award: G2366462802
OpenAlex ID: W2104171741
