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Invisible Middleweight Black Holes Discovered ⚡ экспресс

Original: "Evidence for Intermediate-Mass Black Holes From Microlensing Signatures in CHIME/FRB catalog 2"
arXiv:2605.19653 · 2026-05-19 · CC BY · ⏱ 1 min · High Energy Cosmology General Relativity
Scientists have caught two intermediate-mass black holes distorting signals from fast radio bursts.
Abstract

A method was developed to search for microlensing events in the dynamic spectra of fast radio bursts (FRBs) and applied to data from CHIME/FRB Catalog 2. Two candidates emerged: FRB 20190131D and FRB 20211115A, with gravitational lens masses of [539–609] and [1544–2571] solar masses, respectively, interpreted as evidence for intermediate-mass black holes (IMBHs). If no intervening structures lie along the line of sight, these IMBHs could be isolated and of primordial origin. In that scenario, primordial black holes (PBHs) in these mass windows would make up about 4% of dark matter. If the signals are not genuine lensing, an upper limit on PBHs with masses >300 M☉ is set at ~13% (95% confidence interval). Further FRB observations and a better grasp of their intrinsic emission mechanisms are needed to confirm this method as a tool for detecting (primordial) IMBHs.

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Black holes come in lightweights—born from dying stars—and supermassive ones at galactic cores. The missing intermediate link had been hiding. Fast radio bursts—cosmic signals lasting milliseconds but carrying the energy of days of sunlight—helped crack the case. Think of these bursts as cries from the depths of the universe. When such a cry skims past a massive invisible object, its path bends—spacetime curvature kicks in—and we receive an altered signal. Astronomers studied the frequency prints of two such 'mumbling' bursts and discovered: objects with masses from 500 to 2,500 Suns blocked their path. Without companion stars and far from galactic clusters, they are prime candidates for intermediate-mass black holes. Here's the twist: if no galaxies are nearby, these invisible giants could have been born not from stars, but right after the Big Bang—as primordial black holes. Stephen Hawking suggested they could account for dark matter. Calculations show such holes make up at most 4% of dark matter, but if the signals mislead, the limit rises to 13%. In any case, we are hearing whispers from the first moments of existence.

🎯 A fast radio burst unleashes more energy in a millisecond than the Sun does in a week.

🎬 In sci-fi, primordial black holes are portals to other universes. But their real role may be humbler: invisible bricks of our cosmos.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
black hole dark matter galaxy big bang spacetime curvature spectroscopy
Laws
Friedmann equationsHubble's lawDoppler effectHawking radiationgravitational lensingBekenstein-Hawking entropy
Original: arXiv:2605.19653 · CC BY · bridge42worlds