A black hole is not a frozen void, but a living magnetic engine. Its 'heart'—the accretion disk, pulsates: inhale, matter spirals into the funnel, exhale — magnetic reconnection tears the field lines, and plasma shoots away from the horizon. These events, flux eruption events (FEE), long hid in numerical simulations, eluding telescopes. But now astrophysicists have armed themselves with a 'stethoscope': a convolutional neural network, trained on libraries of GRMHD models, learned to recognize the characteristic patterns of such sighs and translated them into quantities accessible to the interferometer of the Event Horizon Telescope.
Trained on manually labeled images, ResNet-18 achieved near-perfect accuracy (95%), distinguishing details invisible to the human eye. But physicists need not just a detector, but an interpreter. So they trained a random forest — on the same data, but on the output labels of the neural network, and only on parameters measurable in real observations: shadow angular size, fluxes, polarization degree. The cascade worked: it turned out that during an eruption, the shadow noticeably swells (FWHM increases), and linear polarization spikes sharply. But the most unexpected signal is silence: the total flux often does not flare up, but drops. Thus, FEE are not the progenitors of the millimeter flares observed in Sagittarius A*.
These findings are not just a game with data. They chart a course for future observational campaigns. In the images of M87* and Sgr A*, fingerprints of FEE may already be lurking, but they can only be extracted by next-generation interferometers — ngEHT and the space observatory BHEX, whose resolution will rival that of light bending right at the horizon. The next step is to catch the breath in real time: dynamic neural networks trained on time series will link eruptions to the launching of relativistic jets and corona pulsations. And then, perhaps, these magnetic sighs will reveal the answer to the accursed question: does information vanish in a singularity? And does a black hole have 'hair'—contrary to the theorem that John Wheeler forged in debate, and Roger Penrose refined mathematically. Just imagine: one such 'sigh' of M87* lasts 11 days — in that time, a light beam could cross the Solar System from edge to edge. A cosmic arrhythmia that we can now eavesdrop on.
For the supermassive black hole at the center of galaxy M87, one such 'sigh' lasts about 11 days — an instant by astronomical standards, but an eternity for a physicist dreaming to peek beyond the horizon.
If you’re familiar with 'Interstellar', imagine: the astronauts by Gargantua see not only the gravitational lens, but also the accretion disk suddenly warped by a spasm — a magnetic eruption rips it open, hurling plasma at near-light speeds. Alas, at such distance they'd be incinerated before they'd notice.