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Ultralight darkish matter might clarify early black gap formation

April 3, 2025
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Ultralight dark matter could explain early black hole formation
That is an artist’s illustration of a supermassive black gap that’s contained in the dust-shrouded core of a vigorously star-forming “starburst” galaxy. It can finally grow to be a particularly vivid quasar as soon as the mud is gone. The analysis workforce believes that the item, found in a Hubble deep-sky survey, may very well be the evolutionary “lacking hyperlink” between quasars and starburst galaxies. The dusty black gap dates again to solely 750 million years after the massive bang. Credit score : NASA, ESA, and N. Bartmann

A black gap is a area of house the place gravity is so sturdy that nothing, not even mild, can escape. There are two important varieties of black gap; stellar mass and supermassive black holes, they usually differ in dimension, formation, and affect on their host galaxy. Stellar mass black holes, just a few to dozens of occasions the mass of the solar, type from collapsing large stars. Supermassive black holes, however, are hundreds of thousands to billions of occasions extra large and have a tendency to reside within the middle of galaxies and develop by way of accretion and mergers.

The origin of supermassive black holes (SMBHs), particularly these over a billion photo voltaic lots and at excessive redshifts, stays unclear. These objects, as their excessive redshift reveals, are at huge distances from Earth and subsequently exist at among the earliest epochs of the universe. One key formation course of is the direct collapse of cooling atomic fuel clouds with out changing into stars. It’s thought this course of might create large “seed” black gap round 100,000 photo voltaic lots with “heavy” seeds that may develop to a billion photo voltaic lots.

In a paper posted to the arXiv preprint server by a workforce led by Hao Jiao from Cornell College, the workforce explores a course of that will clarify the existence of the SMBHs at such excessive excessive redshifts. On the middle of their speculation is the circulate of ultraviolet radiation that may dissociate hydrogen molecules which forestall fragmentation of the cloud and allow its collapse. In different phrases, they’ve a idea to elucidate how the UV radiation might help create the appropriate situations for the formation of SMBHs within the early universe.

They assume that darkish matter consists of ultra-light wave-like particles, known as “axions,” which work together with electromagnetism by way of specific topological interactions identified mathematically because the Chern-Simons time period. In darkish matter halos, axion subject oscillations can amplify infrared photons by way of power switch from the axion subject to the photons (parametric resonance.) This may additionally result in the emission of ultraviolet radiation both by the thermal power reaching equilibrium or the optically thick halos or by way of a powerful photon cascade from the resonance course of.

The examine reveals that ultralight darkish matter (axions) can generate sufficient UV photons for the direct collapse of black holes by way of the method of parametric resonance. This enables for black gap formation through the earliest durations of the historical past of the universe, with out the necessity for starlight or stellar evolution and will clarify the presence of supermassive black holes at excessive redshifts.

Their mechanism works and is in accordance with a number of fashionable theories, akin to the usual cosmological mannequin (which articulates the construction and evolution of the universe) and with cosmic string seeds (that are theorized as one-dimensional topological defects in spacetime.) Even parts of string idea help the mannequin the place cosmic string loops might assist by seeding halos earlier and making them extra concentrated, growing the probability of their formation.

Extra data:
Hao Jiao et al, Direct Collapse Supermassive Black Holes from Ultralight Darkish Matter, arXiv (2025). DOI: 10.48550/arxiv.2503.19414

Journal data:
arXiv


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