Solar neutrino flux at keV energies
arXiv:1708.02248 · doi:10.1088/1475-7516/2017/12/010
Abstract
We calculate the solar neutrino and antineutrino flux in the keV energy range. The dominant thermal source processes are photoproduction (), bremsstrahlung (), plasmon decay (), and emission in free-bound and bound-bound transitions of partially ionized elements heavier than hydrogen and helium. These latter processes dominate in the energy range of a few keV and thus carry information about the solar metallicity. To calculate their rate we use libraries of monochromatic photon radiative opacities in analogy to a previous calculation of solar axion emission. Our overall flux spectrum and many details differ significantly from previous works. While this low-energy flux is not measurable with present-day technology, it could become a significant background for future direct searches for keV-mass sterile neutrino dark matter.
32 pages, 23 figures. Added several references, a new figure and minor changes to match published version
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- Relic neutrinos at accelerator experiments
- Constraints on Decaying Sterile Neutrinos from Solar Antineutrinos
- Borexino results on neutrinos from the Sun and Earth
- Upper Limits on the Cosmic Neutrino Background from Cosmic Rays
- Axion Helioscopes as Solar Thermometers
- Neutrino astronomy as a probe of physics beyond the Standard Model: decay of sub-MeV - gauge boson dark matter
- Terrestrial Probes of Electromagnetically Interacting Dark Radiation
- Neutrino Emissivities as a Probe of the Internal Magnetic Fields of White Dwarfs
- Probing sub-eV Dark Matter decays with PTOLEMY
- Sensitivity to neutrino-antineutrino transitions for boron neutrinos
- Neutrinos from stars in the Milky Way
- Status and Perspectives of Neutrino Physics
- Detection horizon for the neutrino burst from the stellar helium flash