This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: Johns Hopkins researchers searching the expanse of the universe for the existence of the first black holes are zeroing in on little red dots that may hold the key to the theoretical phenomenon. Using data from the James Webb Space Telescope, researchers from Johns Hopkins have tested whether one specific little red dot, called QSO1, could contain a primordial black hole—a theoretical object that predates the existence of stars, galactic dust particles and heavier elements.
The research could offer insight into how primordial black holes, which astrophysicists have never found direct evidence for, may be formed. The findings are published in the journal Physical Review Letters. "A black hole is an object born from the gravitational death of a star.
Primordial black holes are a very different story," said co-author Valerio De Luca, a postdoctoral researcher in the Department of Physics and Astronomy at Johns Hopkins University. "They come from the physics of the early universe that predates the first stars, when the universe was expanding exponentially in time and space. So the mechanisms for creating primordial black holes are different." Since Stephen Hawking first proposed the idea of primordial black holes in the 1970s, scientists have been working to determine what kind of evidence would be needed to prove their existence and differentiate them from astrophysical black holes.
Astrophysicists have recently turned to swirling, superhot disks of galactic dust particles, energy and gas—the little red dots on JWST images—to find answers. "These little red dots could surround astrophysical black holes, and most probably many of them do, but they could also be primordial black holes, if primordial black holes exist," De Luca said. "So the question becomes, 'Which ones are primordial and how can we tell?'" As a proof of concept, the researchers turned to QSO1, which scientists suspected could contain a primordial black hole based on its age, size and composition.
QSO1 existed just 700 million years after the Big Bang and, unlike other little red dots, is almost entirely made of hydrogen and helium—the first elements that formed during the beginning of the universe—and lacks the heavier elements that formed later in the universe's timeline. A primordial black hole would only be able to grow to QSO1's size and obtain a swirling disk under special circumstances. "There are constraints on primordial black holes from cosmological observations.
There can only be so many primordial black holes in the universe, for example, and there cannot be too many of them in a given cluster," said co-author Loris Del Grosso, a postdoctoral researcher in the Department of Physics and Astronomy. Researchers at Johns Hopkins modeled three scenarios to see if a primordial black hole could possibly develop into a little red dot that is QSO1's size and is surrounded by that concentration of other disks. The most likely scenario: A smaller primordial black hole pulled in and consumed surrounding gas and energy until it grew to be the size of QSO1.
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