Heavy 'Seeds' and Mergers: The Recipe for Black Hole Growth express

Original: "First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes"
arXiv:2604.01123 · 2026-04-01 · CC BY 4.0 · 1 min
Simulations explain how giant black holes managed to grow within just a few hundred million years after the Big Bang.

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The James Webb telescope discovered black holes — so named by John Wheeler, and Karl Schwarzschild described them as a light trap — which, just 500 million years after the Big Bang, already weighed more than a million Suns. It all began with heavy 'seeds' — future black holes with masses of tens of thousands of Suns, born in dense clumps of primordial gas within dark matter scaffolds. These embryos merged like voices in a choir, rapidly building up power. Later, gas absorption provided the main growth. Simulations showed that nearly half of the mass comes from mergers; otherwise, giants like the galaxy GN-z11 wouldn't have had time to grow.

It's like an orchestra: a powerful chord emerges from the fusion of sounds — first the heavy notes of the seeds, then the duets of mergers, and finally the sustained melody of accreting gas. And the cosmic 'chirp' from gravitational waves is the final note.

Interestingly, the seeds probably collapsed directly from gas, skipping the star stage. Calculations promise up to four mergers per year for the LISA observatory — hundreds of times more than previous forecasts.

If space had sound, a black hole merger would sound like a low hum quickly soaring upward — a cosmic 'chirp'.

Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
supermassive black hole growth intermediate mass black hole supermassive black hole formation population iii stars