Astronomers Aaron Smith and Volker Bromm of the University of Texas at Austin, working with Avi Loeb of the Harvard-Smithsonian Center for Astrophysics, have discovered evidence for an unusual kind of black hole born extremely early in the universe. In new research they show that a recently discovered source of intense radiation is likely powered by a “direct-collapse black hole,” a phenomenon predicted by theorists more than a decade ago.
The work was published this month in the journal Monthly Notices of the Royal Astronomical Society.
“It’s a cosmic miracle,” Bromm said, referring to the precise set of conditions present half a billion years after the Big Bang that allowed the behemoths to emerge. “It’s the only time in the history of the universe when conditions are just right” for them to form.
Direct-collapse black holes also may be the solution to a long-standing puzzle in astronomy: How did supermassive black holes form in the early epochs of the universe? There is strong evidence for their existence, as they are needed to power the highly luminous quasars detected in the young universe. However, there are several problems preventing their formation, and the conventional growth process is much too slow.
Astronomers think they know how supermassive black holes weighing in at millions of suns grow in the heart of most galaxies in our epoch. They start from a “seed” black hole, created when an extremely massive star collapses. The seed black hole has the mass of about 100 suns. It pulls in gas from its surroundings, becoming much bigger, and eventually may merge with other seed black holes. The process is called accretion.
The accretion theory does not explain supermassive black holes in extremely distant — and therefore young — quasars. The incredible brightness of quasars, visible across billions of lightyears, comes from matter spiraling into a supermassive black hole, creating jets that shine as beacons across the universe.
These early galaxies may have contained the first generation of stars created after the Big Bang. And although these stars can collapse to form black holes, they don’t work as early quasar seeds. There is no surrounding gas for the black hole to feed on. That gas has been blown away by winds from the hot, newly formed stars.
“Star formation is the enemy of forming massive black holes” in early galaxies, Bromm said. “Stars produce feedback that blows away the surrounding gas cloud.”
For decades, astronomers have called this conundrum “the quasar seed problem.”
Thirteen years ago, Bromm and Loeb came up with an idea to get an early galaxy to form a supermassive seed black hole, by suppressing the otherwise prohibitive energy input from star formation. Astronomers later dubbed this process “direct collapse.”
Begin with a “primordial cloud of hydrogen and helium, suffused in a sea of ultraviolet radiation,” Bromm said. “You crunch this cloud in the gravitational field of a dark matter halo. Normally, the cloud would be able to cool, and fragment to form stars. However, the ultraviolet photons keep the gas hot, thus suppressing any star formation. These are the desired, near-miraculous conditions: collapse without fragmentation! As the gas gets more and more compact, eventually you have the conditions for a massive black hole.”
This set of cosmic conditions is exquisitely sensitive to the time period in the universe’s history — the process does not happen in galaxies today.
Harvard-Smithsonian Center for Astrophysics Communications | February 18, 2015 |
According to Loeb, “The quasars observed in the early universe resemble giant babies in a delivery room full of normal infants. One is left wondering: What is special about the environment that nurtured these giant babies? Typically the cold gas reservoir in nearby galaxies like the Milky Way is consumed mostly by star formation.
“The theory we proposed when Bromm was my postdoc [at Harvard] suggested that the conditions in the first generation of galaxies were different,” he said. “Instead of making many normal stars, these galaxies formed a single supermassive star at their center that ended up collapsing to a seed black hole. Hence the gas in these environments was used to feed this seed black hole rather than make many normal stars.”
Bromm and Loeb published their theory in 2003. “But it was all theoretical back then,” Bromm said.
Bromm is now a professor with postdocs and graduate students of his own, one of whom is Smith.
Smith, Bromm, and Loeb became interested in a galaxy called CR7, identified from a Hubble Space Telescope survey called COSMOS, in a paper led by Jorryt Matthee of Leiden University. Hubble had spied CR7 at 1 billion years after the Big Bang.
David Sobral, then at the University of Lisbon, made follow-up observations of CR7 with some of the world’s largest ground-based telescopes. These uncovered some extremely unusual features in the light signature coming from CR7. Specifically a certain hydrogen line in the spectrum, known as “Lyman-alpha,” was several times brighter than expected. Remarkably, the spectrum also showed an unusually bright helium line.
“Whatever is driving this source is very hot — hot enough to ionize helium,” Smith said.
Bromm agreed. “You need it to be 100,000 K — very hot, a very hard UV source” for that to happen, he said.
These and other unusual features in the spectrum, such as the absence of any detected lines from elements heavier than helium together with the source’s distance — and therefore its cosmic epoch — meant that it could either be a cluster of primordial stars or a supermassive black hole likely formed by direct collapse.
Smith ran simulations for both scenarios using the Stampede supercomputer at UT Austin’s Texas Advanced Computing Center. “We developed a novel code,” Smith said, explaining that his code modeled the system differently than previous simulations. “The old models were like a snapshot; this one is like a movie.”
The type of modeling Smith used is called “radiation hydrodynamics,” Bromm said. “It’s the most expensive approach in terms of computer processing power.”
The new code paid off, though. The star cluster scenario “spectacularly failed,” Smith said, while the direct-collapse black hole model performed well.
Bromm said their work is about more than understanding the inner workings of one early galaxy.
“With CR7, we had one intriguing observation. We are trying to explain it, and to predict what future observations will find. We are trying to provide a comprehensive theoretical framework.”
In addition to Smith, Bromm, and Loeb’s work, NASA recently announced the discovery of two additional direct-collapse black hole candidates based on observations with the Chandra X-ray Observatory.
It seems astronomers are “converging on this model,” for solving the quasar seed problem, Smith said.