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Italian National Institute for Nuclear Physics detects star fusion neutrinos for first time

For the first time ever, scientists at the Gran Sasso National Laboratories of the Italian National Institute for Nuclear Physics have detected neutrinos that were produced within the Sun by the carbon-nitrogen-oxygen cycle. This was something that was theorized back in 1938, but until now, it remained just a theory.

The experiment results, which were published in Nature, state, “Here we report the direct observation, with a high statistical significance, of neutrinos produced in the CNO cycle in the Sun.” These neutrinos were detected using the lab’s state-of-the-art Borexino detector, the same detector that had previously been used to study the primary mechanism of energy production in the Sun, the proton-proton chain.

In order for the Borexino detector to find the neutrinos, the scientists at the lab had to make its core the least radioactive place on Earth. They also spent years advancing liquid-scintillator technology to its absolute limit to prepare it for detections like these.

A look at the onion-like structure of the Borexino sphere

These findings lend truth to the fact that the carbon-nitrogen-oxygen cycle only accounts for about 1% of our Sun’s energy production. However, it is currently believed that in massive stars, this form of energy production is dominant.

Another critical role that neutrinos play in the universe is in dark matter. It is theorized that neutrinos that originated from the Big Bang could account for some of the dark matter in the universe. An asymmetry that lies between neutrinos and their antiparticles may explain why we haven’t been finding more dark matter out there in the universe despite there likely being a lot of it.

Via Italian National Institute for Nuclear Physics

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Nick has a love for technology, cars, and space.