Beyond NGC 1068: New Evidence for Neutrinos from Supermassive Black Holes

In this episode, we dive into the frozen depths of the Antarctic to discuss the latest breakthrough from the IceCube Neutrino Observatory. Building on the historic detection of NGC 1068, the IceCube Collaboration has turned its eyes (or rather, its sensors) to the Southern Hemisphere to search for high-energy neutrinos emitting from X-ray bright Seyfert galaxies.

We explore how researchers used a technique called "stacking" to analyze 14 specific active galaxies. While individual sources like the Circinus Galaxy showed promise but lacked statistical significance on their own, the combined data revealed a compelling excess of neutrino events.

Key Takeaways:

* The Target: The study focused on Seyfert galaxies, where supermassive black holes are obscured by dense dust and gas, making neutrinos—which can pass through this matter—the perfect messenger particles.

* The Method: Using a dataset spanning 2011–2021, the team applied an "Enhanced Starting Track" selection to filter out atmospheric noise in the Southern Sky.

* The Result: By stacking the signals from these galaxies, researchers found a cumulative excess of 6.7 events, reaching a significance level of 3.0 sigma.

* The Implications: This result supports the "disk-corona model," suggesting that cosmic rays are accelerated in the turbulent, magnetized plasma near a black hole, producing neutrinos in environments too dense for gamma rays to escape.

Featured Article

Abbasi, R., et al. (IceCube Collaboration). "Evidence for neutrino emission from X-ray Bright Seyfert Galaxies in the Southern Hemisphere using Enhanced Starting Track Events with IceCube." *Draft version submitted to ApJL*, February 12, 2026. arXiv:2602.10208v1.

Acknowledements: Podcast prepared with Google/NotebookLM. Illustration credits: IceCube Collaboration/NSF