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This month's Challenge Question: Specs & Techs from IHS Engineering360:
A neutrino with an energy of 14 MeV is released from a fusion reaction in the core of the sun and travels on a path directly through Earth. An ideal neutrino detector capable of detecting every neutrino of that energy passing through Earth fails to detect it. Why?
And the answer is:
The neutrino has changed to a different flavor invisible to that detector. The neutrinos released in fusion reactions in the solar core must travel through the extremely dense material of the sun before exiting its atmosphere and travelling across the vacuum of space to Earth. On their journey from the center of the sun to space, neutrinos undergo oscillations and some change from their original electron flavors to muon and tau flavors.
This oscillation effect is the cause of the apparent discrepancy between the amount of neutrinos expected to be emitted from the sun according to the standard solar model and the number of neutrinos actually detected. Early detectors were only picking up between one third and one half of the expected number of neutrinos because they were looking only for electron neutrinos, and couldn’t detect the muon and tau flavors. The Sudbury Neutrino Observatory provided definitive evidence that neutrinos undergo oscillation to different flavors as they travel through the sun.
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