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Phys. Rev. Lett. 97, 191303 (2006) [4 pages]

Can Sterile Neutrinos Be the Dark Matter?

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Uroš Seljak2,1,5, Alexey Makarov1, Patrick McDonald3, and Hy Trac4
1International Center for Theoretical Physics, Trieste, Italy
2Physics Department, Princeton University, Princeton, New Jersey 08544, USA
5Institute for Theoretical Physics, University of Zurich, Winterthur Strasse 190, 8057 Zurich, Switzerland
3Canadian Institute for Theoretical Astrophysics, University of Toronto, ON M5S 3H8, Canada
4Princeton University Observatory, Princeton, New Jersey 08544, USA

Received 20 February 2006; revised 22 September 2006; published 8 November 2006

We use the Ly-α forest power spectrum measured by the Sloan Digital Sky Survey and high-resolution spectroscopy observations in combination with cosmic microwave background and galaxy clustering constraints to place limits on a sterile neutrino as a dark matter candidate in the warm dark matter scenario. Such a neutrino would be created in the early Universe through mixing with an active neutrino and would suppress structure on scales smaller than its free-streaming scale. We ran a series of high-resolution hydrodynamic simulations with varying neutrino masses to describe the effect of a sterile neutrino on the Ly-α forest power spectrum. We find that the mass limit is ms>13  keV at 95% C.L. (9 keV at 99.9%), which is above the upper limit allowed by x-ray constraints, excluding this candidate from being all of the dark matter in this model.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.97.191303
DOI:
10.1103/PhysRevLett.97.191303
PACS:
95.35.+d, 14.60.St, 98.62.Ra