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Scientists have traced the origins of essentially the most huge black gap merger ever noticed, revealing how two “impossible” giants could have fashioned regardless of long-standing assumptions that such objects mustn’t exist.
These black holes had been thought-about “forbidden” as a result of stars of that dimension had been thought to blow themselves aside in extraordinarily highly effective explosions, forsaking no remnant that would collapse right into a black gap.
The findings also suggest that black holes can form more efficiently than scientists thought, which could transform our understanding of how the universe’s first stars and black holes gave rise to today’s supermassive black holes.
Why heavy black hole mergers matter
Black hole collisions have become one of the most important tools for understanding the universe.
“Black hole mergers allow us to observe the universe not through light, but through gravity — via gravitational waves produced by the distortion of space and time as black holes spiral together and merge,” Ore Gottlieb, a professor on the Center for Computational Astrophysics who led the work, instructed Live Science in an e-mail. Gravitational waves supply a uncommon view into areas of area the place gravity is so excessive that not even gentle can escape. From the form of the sign alone, scientists can infer the plenty and spins of the merging objects and reconstruct how they fashioned.
These observations check Einstein’s principle of basic relativity the place its predictions are essentially the most demanding, as a result of the space-time curvature round merging black holes pushes the speculation to its limits. Events involving the heaviest black holes additionally reveal how huge stars lived and died throughout cosmic time and the way early black holes grew into the monsters that sit on the facilities of galaxies right now.
The most huge black gap merger ever detected
Stars in this range usually tear themselves apart through violent supernova explosions, leaving nothing behind. Yet GW231123 housed not one, but two such objects — and both showed signs of spinning at extreme rates. The event involved “two of the most rapidly spinning black holes, indicating a rare formation channel of massive and rapidly spinning black holes, which were not supposed to exist,” Gottlieb said.
To unravel how such black holes could form, the team created detailed, three-dimensional simulations, starting from the life of an extremely massive star. The model followed a helium core about 250 times the mass of the sun as it burned fuel, collapsed, and formed a newborn black hole. Earlier theories assumed such a star would collapse in one piece, leaving a black hole as heavy as the original core. But the new study shows this is not always the case.
Solving the impossible
Gottlieb and colleagues found that rapid rotation changes everything.
“We showed that if the star rotates rapidly, it forms an accretion disk around the newly born black hole,” Gottlieb explained. “Strong magnetic fields generated within this disk can drive powerful outflows that expel part of the stellar material, preventing it from falling into the black hole.” Instead of swallowing the entire core, the young black hole loses access to much of the surrounding matter as magnetic forces blast material into space.
This mechanism reduces the final mass of the remnant, pushing it down into the mass gap — a region previously thought unreachable. “As a result, the final black hole mass can be significantly reduced, landing within the mass gap, a range previously thought to be inaccessible,” Gottlieb said.
The simulations also naturally produced a link between the mass and spin of the resulting black hole. Strong magnetic fields extract angular momentum, thus slowing the black hole while ejecting more mass. Weaker fields leave a more massive, faster-spinning object. This relationship closely matches the properties inferred for the two black holes in GW231123. One would form in a star with moderate magnetic fields, and the other would form in a star with weaker ones, creating a pair with different final masses and spins — exactly what the gravitational wave signal suggests.
What these discoveries mean for gravity and cosmic history
Extreme events like GW231123 stretch general relativity to its breaking point.
“The tremendous curvature of space and time probes general relativity deep in its most extreme strong field regime, enabling us to test whether Einstein’s equations remain accurate when gravity is at its most extreme,” Gottlieb noted.
If similar events happened frequently in the early universe, they would have shaped the growth of the first black holes. Such mergers “imply that massive black holes can form more efficiently than current stellar models predict,” Gottlieb said. “This would affect our understanding of how the first generation of stars and black holes seeded the supermassive black holes we observe in galaxies today.”
The team’s work points to a new formation pathway for massive black holes and predicts specific patterns astronomers can search for. “Our work opens a new window to black hole formation within the mass gap, predicting first-generation black holes (without previous mergers) at all masses,” Gottlieb said. Future gravitational-wave detections will test whether the mass-spin correlation found in the simulations holds across many events.
“As we detect more massive black hole binaries, we will be able to test the predicted correlation on this population,” Gottlieb said. These discoveries may reveal whether GW231123 is a cosmic rarity or the first clear sign of a hidden population of massive, rapidly spinning black holes.
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