
arXiv: 0806.4273
We consider sterile neutrinos with rest masses ~0.2 GeV. Such sterile neutrinos could augment core collapse supernova shock energies by enhancing energy transport from the core to the vicinity of the shock front. The decay of these neutrinos could produce a flux of very energetic active neutrinos, detectable by future neutrino observations from a galactic supernova. The relevant range of sterile neutrino masses and mixing angles can be probed in future laboratory experiments.
5 pages
Nuclear and High Energy Physics, Supernova, 5106 Nuclear and Plasma Physics (for-2020), Particle and Plasma Physics (for), FOS: Physical sciences, 0201 Astronomical and Space Sciences (for), 51 Physical sciences (for-2020), Astrophysics, Atomic, Particle and Plasma Physics, astro-ph, 0105 Mathematical Physics (for), Nuclear, Mathematical Physics, 5107 Particle and High Energy Physics (for-2020), 51 Physical Sciences (for-2020), Astrophysics (astro-ph), Molecular, Nuclear & Particles Physics (science-metrix), Nuclear & Particles Physics, 49 Mathematical sciences (for-2020), Supernova shock, 0202 Atomic, Sterile neutrinos, Astronomical and Space Sciences
Nuclear and High Energy Physics, Supernova, 5106 Nuclear and Plasma Physics (for-2020), Particle and Plasma Physics (for), FOS: Physical sciences, 0201 Astronomical and Space Sciences (for), 51 Physical sciences (for-2020), Astrophysics, Atomic, Particle and Plasma Physics, astro-ph, 0105 Mathematical Physics (for), Nuclear, Mathematical Physics, 5107 Particle and High Energy Physics (for-2020), 51 Physical Sciences (for-2020), Astrophysics (astro-ph), Molecular, Nuclear & Particles Physics (science-metrix), Nuclear & Particles Physics, 49 Mathematical sciences (for-2020), Supernova shock, 0202 Atomic, Sterile neutrinos, Astronomical and Space Sciences
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