Measuring the cosmological background of relativistic particles with WMAP

Details Measuring the cosmological background of relativistic particles with WMAP Measuring the cosmological background of relativistic particles with WMAP

2003-02-17

arxiv.org/abs/astro-ph/0302337v2

Phys.Rev.D67:123005,2003

Astronomy and Astrophysics

Astrophysics

5 pages, 2 figures (1 new figure). Version to be published

Scientific paper

10.1103/PhysRevD.67.123005

We show that the first year results of the Wilkinson Microwave Anisotropy Probe (WMAP) constrain very efficiently the energy density in relativistic particles in the universe. We derive new bounds on additional relativistic degrees of freedom expressed in terms of an excess in the effective number of light neutrinos Delta N_eff. Within the flat LambdaCDM scenario, the allowed range is Delta N_eff < 6 (95% CL) using WMAP data only, or -2.6 < Delta N_eff < 4 with the prior H_0= 72 \pm 8 km/s/Mpc. When other cosmic microwave background and large scale structure experiments are taken into account, the window shrinks to -1.6 < Delta N_eff < 3.8. These results are in perfect agreement with the bounds from primordial nucleosynthesis. Non-minimal cosmological models with extra relativistic degrees of freedom are now severely restricted.

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