Cosmological Implications of Light Sterile Neutrinos produced after the QCD Phase Transition
arXiv:1411.2690 · doi:10.1103/PhysRevD.91.063502
Abstract
We study the production of sterile neutrinos in the early universe from shortly after the QCD phase transition in the absence of a lepton asymmetry while including finite temperature corrections to the mass and decay constant . Sterile neutrinos with masses produced via this mechanism freeze-out at with a distribution function that is highly non-thermal and features a sharp enhancement at low momentum thereby making this species \emph{cold} even for very light masses. Dark matter abundance constraints from the CMB and phase space density constraints from the most dark matter dominated dwarf spheroidal galaxies provide upper and lower bounds respectively on combinations of mass and mixing angles. For , the bounds lead to a narrow region of compatibility with the latest results from the line. The non-thermal distribution function leads to free-streaming lengths (today) in the range of $\sim \mbox{few kpc}$ consistent with the observation of cores in dwarf galaxies. For sterile neutrinos with mass that are produced by this reaction, the most recent accelerator and astrophysical bounds on combined with the non-thermal distribution function suggests a substantial contribution from these sterile neutrinos to .
32 pages, 8 figures, new references and corrected typos
References in corpus (16)
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Dark-matter sterile neutrinos in models with a gauge singlet in the Higgs sector
- Too Big to Fail in the Local Group
- Resonantly-Produced 7 keV Sterile Neutrino Dark Matter Models and the Properties of Milky Way Satellites
- Phase transitions in the early and the present Universe
- Search for a Light Sterile Neutrino at Daya Bay
- The emptiness of voids: yet another over-abundance problem for the LCDM model
- Constraints on dark matter particles from theory, galaxy observations and N-body simulations
- Clustering properties of a sterile neutrino dark matter candidate
- Small-scale structure formation properties of chilled sterile neutrinos as dark matter
- 3.5 keV X-rays as the "21 cm line" of dark atoms, and a link to light sterile neutrinos
- Nearly degenerate heavy sterile neutrinos in cascade decay: mixing and oscillations
- Free streaming in mixed dark matter
- Constraining Sterile Neutrinos Using Reactor Neutrino Experiments
- Space-time evolution of heavy sterile neutrinos in cascade decays
- Daughters mimic sterile neutrinos (almost!) perfectly
Cited by in corpus (9)
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- keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
- Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling
- The surprising influence of late charged current weak interactions on Big Bang Nucleosynthesis
- Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures
- A short survey of matter-antimatter evolution in the primordial universe
- Warm Dark Matter from Higher-Dimensional Gauge Theories