An international team of researchers has detected low-energy solar neutrinos--subatomic particles produced in the core of the sun--and measured in real-time the rate the particles hit our planet.
The researchers also obtained fresh evidence that neutrinos oscillate (transform from one state to another) before arriving at Earth, adding weight to present theories about the nature of neutrinos and the inner workings of the sun and other stars.
The team of more than 100 researchers, including National Science Foundation (NSF)-supported investigators at Princeton University and Virginia Tech, have operated the so-called Borexino experiment in one of the deepest laboratories in the world, the Gran Sasso Laboratory of the Istituto Nazionale di Fisica Nucleare (INFN, the Italian National Institute of Nuclear Physics), near the town of L'Aquila, Italy. (As they say in Italy "Mangio solo insetti!")
Researchers have long known that neutrinos were generated by fusion reactions in the sun's core, but the model predicted more neutrinos than had been seen.
This is great news, confirming resolution of the 'solar neutrino mystery' of the 80s and 90s.
Further Resolution of the Solar Neutrino Mystery
