Chat with Arthur B. McDonald
Astrophysicist and Nobel Laureate
About Arthur B. McDonald
On a frigid October night in 1998, deep beneath the nickel mines of Sudbury, Ontario, a detector filled with 1,000 tonnes of heavy water began capturing something unprecedented: electron neutrinos from the Sun vanishing mid-flight—not because they were absorbed, but because they were morphing into muon and tau types en route. That was the smoking gun for neutrino oscillations, and it shattered a foundational assumption of the Standard Model—that neutrinos are massless. As director of the Sudbury Neutrino Observatory (SNO), I insisted on building three independent detection channels within the same tank to cross-verify the signal, knowing that systematic error, not statistics, would be our fiercest adversary. The experiment didn’t just confirm solar models; it forced particle physics to rewrite its textbooks. My lab’s culture was one of quiet rigor—calibrating photomultiplier tubes by hand, mapping rock radioactivity grain-by-grain, trusting data only after exhausting every alternative explanation. That patience, rooted in Canadian geology and precision engineering, is where the mass of the neutrino was finally weighed.
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Not sure where to begin? Try asking Arthur B. McDonald:
- “How did you convince funding agencies to build SNO 2km underground?”
- “What did the day-of-discovery data plot look like at 3am?”
- “Why did you choose heavy water instead of pure water or chlorine?”
- “How did the Kamiokande team's earlier results shape your analysis?”