WMAP, neutrino degeneracy, and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation

2003/11/30 by Christopher Gordon, Chris Gordon, Karim A. Malik · 54 citations
Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #CMB cold spot #Cosmic microwave background #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Degeneracy (biology) #Degenerate energy levels #Inflation (cosmology) #Lepton #Lepton number #Neutrino #Non-Gaussianity #Nuclear physics #Nucleosynthesis #Particle physics #Physics #Quantum mechanics #Supernova #Theoretical physics #astro-ph #hep-ph

paper · pdf · doi:10.1103/physrevd.69.063508

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 69(6) (American Physical Society) · 8 pages. Minor changes to text, references added, matches version to appear in PRD

arxiv created 2004/03/05 · openalex publication_date 2004/03/16 · arxiv updated 2011/05/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

In the curvaton model of inflation, where a second scalar field, the ``curvaton,'' is responsible for the observed inhomogeneity, a nonzero neutrino degeneracy may lead to a characteristic pattern of isocurvature perturbations in the neutrino, cold dark matter and baryon components. We find that the current data can only place upper limits on the level of isocurvature perturbations. These can be translated into upper limits on the neutrino degeneracy parameter. In the case that lepton number is created before curvaton decay, we find that the limit on the neutrino degeneracy parameter is comparable with that obtained from big-bang nucleosynthesis. For the case that lepton number is created by curvaton decay we find that the absolute value of the non-Gaussianity parameter, |f_nl|, must be less than 10 (95% confidence interval).

Citations

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