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- W2000632844 abstract "If the source of the reported 3.5 keV x-ray line is a sterile neutrino, comprising an $mathcal{O}(1)$ fraction of the dark matter (DM), then it exhibits the property that its mass times mixing angle is $ensuremath{sim}text{ }text{few}ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}2}text{ }text{ }mathrm{eV}$, a plausible mass scale for the active neutrinos. This property is a common feature of Dirac neutrino mixing. We present a framework that dynamically produces light active and keV sterile Dirac neutrinos, with appropriate mixing angles to be the x-ray line source. The central idea is that the right-handed active neutrino is a composite state, while elementary sterile neutrinos gain keV masses similarly to the quarks in extended technicolor. The entire framework is fixed by just two dynamical scales and may automatically exhibit a warm dark matter (WDM) production mechanism---dilution of thermal relics from late decays of a heavy composite neutrino---such that the keV neutrinos may comprise an $mathcal{O}(1)$ fraction of the DM. In this framework, the WDM is typically quite cool and within structure formation bounds, with temperature $ensuremath{sim}text{ }text{few}ifmmodetimeselsetexttimesfi{}{10}^{ensuremath{-}2}{T}_{ensuremath{nu}}$ and free-streaming length $ensuremath{sim}text{ }mathrm{few}text{ }text{ }mathrm{kpc}$. A toy model that exhibits the central features of the framework is also presented." @default.
- W2000632844 created "2016-06-24" @default.
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- W2000632844 date "2014-08-25" @default.
- W2000632844 modified "2023-10-15" @default.
- W2000632844 title "Dynamical framework for KeV Dirac neutrino warm dark matter" @default.
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- W2000632844 doi "https://doi.org/10.1103/physrevd.90.045030" @default.
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