# Johns Hopkins model links Webb's QSO1 black hole to a primordial seed growing by gas accretion

- Published: 2026-11-05 21:28 UTC
- Section: Sky & Space › Astronomy
- Tags: Little Red Dots, primordial black holes, QSO1, Abell 2744, James Webb Space Telescope, supermassive black holes, gas accretion, Johns Hopkins University, Eddington limit
- URL: https://realtech.media/news/rt-70b696085066056619cb95eb_johns_hopkins_model/

**A theoretical study compared three formation routes for black holes in Webb's Little Red Dots; gas growth of a seed of about 1,000 solar masses fits QSO1 best.**

![Johns Hopkins model links Webb's QSO1 black hole to a primordial seed growing by gas accretion](https://sgzwpqqelzmajkcubgkl.supabase.co/storage/v1/object/public/rt-media/2026/11/db482ef961a8b2fe.webp)
*scinexx*

Researchers at Johns Hopkins University led by Valerio De Luca have modelled three ways in which black holes could form in the Little Red Dots, compact high-redshift sources found by the James Webb Space Telescope. The work, published in Physical Review Letters, is based on previously released Webb data [1]. Some of these objects appear to host black holes much heavier than their stellar content would suggest when compared with local scaling relations [1].

The test case was Abell 2744-QSO1 (QSO1), a source magnified by the gravitational lens of a foreground galaxy cluster. Its light dates from about 700 million years after the Big Bang. Its central black hole has roughly 50 million solar masses, while the surroundings contain less than one hundredth of the solar fraction of heavier elements [1].

## Direct formation and mergers

In the first scenario, a black hole of such mass would form directly in the early Universe. According to the calculations, this is excluded by cosmic microwave background μ-distortion limits: the required strong density fluctuations would have left measurable traces [1]. Primordial black holes that remain allowed as seeds have at most about 1,000 solar masses.

The second route is hierarchical merging of such lighter seeds. It can operate depending on the merger history, but the growing black holes would have to stay inside very massive dark matter halos despite the recoil from collisions. In the model, such halos are too rare at high redshift to explain the observed abundance of Little Red Dots [1].

## Growth by gas accretion

The third route proved the most promising in the calculations: a seed of about 1,000 solar masses accretes gas. With sufficiently efficient inflow, it could reach many millions of solar masses by the epoch of QSO1. At times the modelled accretion rate exceeds the classical Eddington limit [1].

The low metallicity of QSO1 constrains this path. Stars forming from the infalling gas would produce heavier elements, so in the suitable models no more than about one percent of the inflowing gas turns into stars [1]. The authors tracked metallicity jointly with accretion and identified regions of parameter space that reproduce the observed properties of the Little Red Dots [1].

The result is a possible evolutionary path, not evidence that primordial black holes exist. Other scenarios, including the collapse of early stars or of very massive gas clouds, remain under discussion. Further observations are needed to show how common a primordial origin could be.

## Sources

1. [Physical Review Letters](https://doi.org/10.1103/6y1w-87pd)
2. [scinexx](https://www.scinexx.de/news/kosmos/rote-punkte-im-weltraum-koennten-urzeitliche-schwarze-loecher-verbergen)

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Source: RealTech, realtech.media — https://realtech.media/news/rt-70b696085066056619cb95eb_johns_hopkins_model/