2026 Nobel Prize in Physics

Those cosmic neutrinos that help us understand the mechanisms of black holes

Francis Halzen is a scientist who has devoted his career to studying the most abundant, yet also the most elusive, particles in the universe

Il fisico delle particelle belga-americano Francis Halzen dell’Università del Wisconsin-Madison, vincitore del Premio Nobel per la Fisica 2026, parla del suo lavoro nel progetto IceCube per il rilevamento dei neutrini in Antartide ad Alexandria, in Virginia (Stati Uniti), il 12 luglio 2018, in un fotogramma tratto da un video.    (REUTERS/via Reuters TV)

3' min read

Translated by AI
Versione italiana

3' min read

Translated by AI
Versione italiana

The 2026 Nobel Prize in Physics has been awarded to Francis Halzen, a scientist who has dedicated his career to the study of cosmic neutrinos – the most abundant, yet also the most elusive, particles in the universe. Thanks to the IceCube detector, built at the South Pole using a cubic kilometre of ice at a depth of over two kilometres, Halzen and his numerous collaborators have pioneered neutrino astronomy, which enables us to understand how supermassive black holes at the centres of active galaxies accelerate the high-energy particles that constantly bombard us – particles we call cosmic rays.

Un tabellone indica che Francis Halzen è stato proclamato vincitore del Premio Nobel per la Fisica 2026 durante una conferenza stampa tenutasi presso l’Accademia Reale Svedese delle Scienze a Stoccolma, in Svezia, il 6 ottobre 2026. (Agenzia di stampa TT/Christine Olsson/via REUTERS)

In fact, the citation for the prize reads: “for decisive contributions to the IceCube Neutrino Observatory and to the discovery of high-energy neutrinos of astrophysical origin”.

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Born and brought up in Belgium, Francis Halzen graduated from the University of Louvain in 1966. After spending a couple of years at CERN, he visited the University of Wisconsin in 1971 and decided to stay there to build his career. Despite having spent over half a century in the United States, he has retained a strong Flemish accent. It was impossible not to notice it during the telephone call in which Halzen answered journalists’ questions. He made no secret of the fact that he was in Italia, where, after attending the Bergamo Festival on Sunday, he stayed on to work on a future project which, perhaps, thanks to the Nobel Prize, will have a better chance of being approved.

Mark Pearce, chair of the Nobel Committee at the Stockholm Academy, said, “Francis Halzen led an international team of researchers and engineers who have provided us with an extraordinary tool”, adding that “His tenacity and scientific vision have paved the way for a new kind of astronomy.”

In fact, looking back at the key milestones in the history of the IceCube Neutrino Observatory, we find that Halzen first presented the plans for this observatory in 1988, envisaging a huge structure buried deep within the Antarctic ice, capable of detecting the passage of elusive neutrinos.

The observatory makes use of a fundamental property of neutrinos: that they produce a flash of light when they interact with an atomic nucleus, a signal that can be detected by sensors embedded in the enormous volume of super-transparent ice.

Building IceCube was an incredible feat of Antarctic logistics. Ultra-pure boiling water carved out shafts through kilometres of ice into which the detectors were lowered; once in place, they were covered with water and immediately encased in ice.

The first neutrinos were detected in 2011, and by 2013 it was already certain that they were of cosmic origin – that is, not produced in our atmosphere. The journal *Science* immediately named it ‘Breakthrough of the Year’. In previous years, solar neutrinos and those produced by the explosion of supernova 1987A had already been detected. Both discoveries were recognised with the Nobel Prize, but this time it is not a single object, however important it may be. IceCube observes the entire sky. In fact, it is not the sky above Antarctica, but rather the one on the other side of the Earth; this is because, to avoid the troublesome neutrinos produced by cosmic particles in the atmosphere, IceCube uses the Earth as a protective shield. They know they’re on safe ground: neutrinos are particles that have absolutely no desire to interact with matter. Originating from the most remote regions of the cosmos, neutrinos are often described as ‘ghostly’ because they are extremely elusive and can pass through any kind of matter without undergoing any changes.

A characteristic that enables them to travel through intergalactic space, but which makes them extremely difficult to detect. In my career as a gamma-ray astronomer, I have often had the opportunity to search for the source of particularly significant events detected by IceCube. In fact, neutrinos and gamma rays are produced together by processes occurring in the vicinity of the supermassive black holes that dominate the most active and luminous galaxies. These same processes are also responsible for the acceleration of ultra-high-energy cosmic rays; however, as these are charged particles, they are deflected by magnetic fields and lose all trace of their origin.

Gamma rays and neutrinos, on the other hand, travel in a straight line, and their combination has made it possible to identify the sources of the universe’s ‘ghosts’.

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