A Real Time Detector for Low Energy Neutrinos
Borexino is a particle physics experiment performed by an international collaboration in the “Hall C” of the Laboratori Nazionali del Gran Sasso (LNGS). The Borexino physics program is centered on solar neutrino, but also includes other relevant topics in low background neutrino detection (including geoneutrinos) and underground physics.
The Borexino detector is a large, low background liquid scintillator detector designed to reveal low energy (sub-MeV) neutrinos in real time. It was built with the main goals of performing solar neutrinos spectroscopy and to measure the 7Be neutrino flux from the Sun.
The very low energy threshold needed to achieve such goals in turn required an extreme radiopurity of the detector (at least 10 orders of magnitude better than in typical natural conditions). Nothing is standard in Borexino: all detector parts and components had to be developed ad hoc, with all involved materials carefully selected for radiopurity (measurements were made with germanium detectors and mass spectrometers). Everything had to go through clean rooms (five were built around the detector). The inside of the detector itself have been equipped as a clean room. The welds were TIG in nitrogen or argon atmosphere, all surfaces were pickled and passivated, the nitrogen for stripping was cryogenically purified, etc.
A Borexino prototype, called the Counting Test Facility (CTF), has been built and operated in the Hall C of LNGS between 1994 and ’96. This (now dismantled) detector demonstrated the achievement of ultra-low count rates (radiopurity of the order of 10-16g/g of 238U equivalent) on the several-ton scale.
The Borexino detector have been built on the CTF experience. Construction have been completed on May 15, 2007. The first data acquisition (DAQ) run with the full detector was started on May 16, 2007. The last DAQ run (#36744) have been stopped on Oct 7, 2021 @ 11:26 am CET, and the detector decommissioning has begun.
The extraordinary radiopurity achieved by Borexino (unprecedented for such a large detector), further improved over the years, have made it possible to accomplish not only its primary goals but also to produce many other interesting results both within and beyond the Standard Model of particle physics.
A selection of the experimental data acquired and analysed by the Borexino collaboration for some of our publications has been made freely available as “Open Data”.
For more information and details please refer to these articles:
- “The Borexino detector at the Laboratori Nazionali del Gran Sasso”
(detailed tech. description. Does not include latest improvements)
- Technologies of the Borexino experiment: Introduction
- Science and Technology in very low energy neutrinos physics with Borexino
- Why and how the Sun and the stars shine
(general description, scientific and historical notes)
- Borexino General Meeting on Dec 2021 – Special Open Session
(recollection of history and achievements of Borexino)
- How the Sun and the Stars shine