Structure Formation with Decaying Neutrinos
arXiv:astro-ph/9411098 · doi:10.1103/PhysRevD.51.2669
Abstract
We consider the effects of a massive, unstable neutrino on the evolution of large--scale structure and anisotropies in the cosmic microwave background. Comparison with large--scale structure data allows us to rule out a wide range of masses and lifetimes for such neutrinos. We also define a range of masses and lifetimes which delay matter--radiation equality and improve the agreement with the data of Cold Dark Matter models with critical density.
13 pages, compressed uuencoded self-unpacking postscript file with 5 figures and 1 table (included)
References in corpus (12)
- Reconstructing the linear power spectrum of cosmological mass fluctuations
- On Determining the Spectrum of Primordial Inhomogeneity from the COBE DMR Sky Maps: II. Results of Two Year Data Analysis
- Refined Big Bang Nucleosynthesis Constraints on and
- Dark Matters in Axino Gravitino Cosmology
- Is a Massive Tau Neutrino Just What Cold Dark Matter Needs?
- Primordial Nucleosynthesis with a Decaying Tau Neutrino
- Dark Matter and Structure Formation with Late Decaying Particles
- Constraints on Dirac Neutrinos from SN 1987A
- Massive Tau Neutrino and SN 1987a
- Supersymmetric Singlet Majorons and Cosmology
- Neutrino Decay in the Doublet Majoron Model
- Stability of Neutrinos in the Singlet Majoron Model
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- Neutrino Masses in Astrophysics and Cosmology
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- A New Astrophysical Constraint on Radiatively Decaying Neutrinos
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