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: If you want to understand the origins of black holes, Yale astronomers say, you need to look beyond the centers of galaxies and start searching in the nooks and crannies. That's where you'll find the "wanderers"—black holes whose journeys may tell the story of how the first black holes formed.
In a new study published in The Astrophysical Journal Letters, astronomers Emma Jane Weller and Priyamvada Natarajan from Yale and Colin Burke from the University of North Texas found that black holes—which are normally located at the centers of galaxies—can be displaced by galactic mergers and wander far from their original locations for billions of years. This process is even more pronounced in smaller galaxies, where there is less gravity pulling a wandering black hole toward the center. "Our results show that considering wandering black holes, in addition to centered black holes, is essential for understanding the origins and dynamics of massive black holes and the histories of their host galaxies," said Weller, who led the research and is an astronomy student in Yale's Graduate School of Arts and Sciences.
The earliest black holes are thought to have originated from "seeds" in the young universe. Some theories propose that the first stars in the universe left behind relatively "light" seeds (smaller black holes); other theories propose that "heavy" seeds (larger black holes) formed even earlier, via processes such as the direct collapse of pristine gas. Natarajan, the Joseph S. and Sophia S.
Fruton Professor of Astronomy and professor of physics in Yale's Faculty of Arts and Sciences, and Weller's thesis adviser, is a leading proponent of the "heavy seeds" theory. "What is exciting about our findings is that black holes seem to remember more than the circumstances of their birth," Natarajan said. "Their present-day locations carry the imprint of everything that has happened to their host galaxies.
By separating black holes at galactic centers from those that are wandering, we can begin to disentangle these two histories." For the study, the researchers used ASTRID, a cosmological simulation that follows the evolution of dark matter, gas, stars and black holes. The team examined galaxies with stellar masses ranging from 10 million to 1 trillion times the mass of the sun, tracing their evolution across approximately 12.6 billion years. One important feature of the ASTRID simulation is that it does not artificially pin black holes to the centers of their galaxies.
Instead, it models the gravitational forces that cause black holes to move through their surroundings and gradually sink toward their galactic centers. This enabled the researchers to distinguish between centered black holes and wanderers. "Some of the universe's most revealing black holes may be the ones that have wandered away," Natarajan said.
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