In the early hours of February 13, 2023, a neutrino struck the ARCA detector on the floor of the Mediterranean Sea. It carried 220 petaelectronvolts of energy — roughly 100,000 times more than the Large Hadron Collider can produce. At 220 PeV, it exceeds anything previously detected by a factor of 20 or more.
For two years, physicists puzzled over KM3-230213A. Then, in February 2026, a team from the University of Massachusetts Amherst published a paper in Physical Review Letters proposing an answer: the particle came from an exploding primordial black hole. If correct, it would be the first observational evidence of Hawking radiation — a theoretical prediction Stephen Hawking made fifty years ago, that black holes slowly evaporate by emitting radiation. A confirmed detection would be a genuine Nobel candidate.
The detection is real. The interpretation is not settled.
The UMass Amherst team, led by assistant professors Michael Baker and Andrea Thamm and postdoctoral researcher Joaquim Iguaz Juan, argues that the black hole in question was not a conventional astrophysical black hole but a quasi-extremal primordial black hole — one carrying a small electric charge under a previously unknown dark force. In this state, it would have spent most of its lifetime dormant, then rapidly discharged in an explosion that produced the ultra-high-energy neutrino KM3NeT caught. The model has a striking implication: if this interpretation holds, primordial black holes could constitute all of the observed dark matter in the universe.
The energy scale is the central fact of this story. 220 PeV is not a rounding error or a marginal measurement — it is a particle carrying more energy than any accelerator on Earth can produce by three orders of magnitude. The LHC tops out around 10 PeV (10,000 TeV). The proposed Future Circular Collider, if built, might reach 100 TeV — still three orders of magnitude short of 220 PeV. KM3NeT, deployed at a depth of 2,500 to 3,500 meters in the Mediterranean, sits in the only location on Earth sensitive enough to catch the cascade of light produced when such a particle interacts with seawater. IceCube, the South Pole detector that won the 2015 Nobel Prize for neutrino astronomy, maxes out at roughly 10 PeV — it cannot see the regime KM3-230213A inhabits.
The detector was running at roughly 10 percent capacity when it made the catch. KM3NeT's full array is planned at over 200 detection units; in February 2023 it had 21. Even at partial strength, the detector recorded 28,000 photons in a two-microsecond window, saturating a quarter of its photomultiplier tubes. This was not a borderline signal — it was a blunt instrument hitting a loud target.
What the PRL paper adds is the theoretical scaffolding. The authors propose that KM3-230213A was generated by the annihilation of an electron-positron pair produced in the final moments of a charged primordial black hole's evaporation. The model invokes new physics beyond the Standard Model — a dark U(1) symmetry and a mechanism for how primordial black holes could carry and shed charge. This is where the caution enters. The dark matter interpretation in particular depends on the existence of an entirely new particle physics sector that has not been independently confirmed.
The paper's own framing is careful: the quasi-extremal PBH model explains the data, but it is not the only possible explanation. Other ultra-high-energy neutrino sources — active galactic nuclei, gamma-ray bursts, starburst galaxies — have not been definitively ruled out for this event. The neutrino arrived from a direction with no known strong astrophysical source (RA=94.3°, dec.=-7.8°), which the authors cite as consistent with a primordial black hole origin, but that absence of a conventional source is also consistent with gaps in surveys of that sky region.
Replication is the test. KM3NeT is currently expanding toward its full sensitivity. IceCube's South Pole upgrade, funded by the NSF and targeting the 2025-2026 drilling season, will add more sensitive instrumentation at energies closer to what IceCube can actually see — not quite 220 PeV but better calibrated than the current array. If KM3NeT detects another event in this energy range from a similar direction, the statistical weight shifts. One event, however dramatic, is a candidate. Two is a population. That second catch is not guaranteed — the authors estimate primordial black hole explosions might occur roughly once per decade, which means the window for a rapid replication may be measured in years, not months.
The story for type0 readers is this: a neutrino detector caught something that should not exist according to known particle physics, and a careful paper explains it with a new form of black hole that also happens to solve the dark matter problem. The energy scale alone makes this worth watching — it is the kind of result that forces physicists to reconsider what they thought they understood about where ultra-high-energy cosmic rays come from. Whether the primordial black hole interpretation survives contact with peer review is a question for the next few years, not the next few weeks.
For now, the honest version of the headline is: physicists think they may have seen a black hole explode. That is already more interesting than most things that happen in a given week.
UMass Amherst announcement: https://www.umass.edu/news/article/did-we-just-see-black-hole-explode-physicists-umass-amherst-think-so-and-it-could
KM3NeT event page: https://www.km3net.org/km-3230213a-full-page/
arXiv preprint: https://arxiv.org/abs/2505.22722
PRL paper: https://journals.aps.org/prl/abstract/10.1103/r793-p7ct