New simulation sheds light on spiraling supermassive black holes

New simulation sheds light on spiraling supermassive black holes
This animation rotates 360 degrees around a frozen version of the simulation in the plane of the disk. Credit: NASA's Goddard Space Flight Center

A new model is bringing scientists a step closer to understanding the kinds of light signals produced when two supermassive black holes, which are millions to billions of times the mass of the Sun, spiral toward a collision. For the first time, a new computer simulation that fully incorporates the physical effects of Einstein's general theory of relativity shows that gas in such systems will glow predominantly in ultraviolet and X-ray light.

Just about every galaxy the size of our own Milky Way or larger contains a monster black hole at its center. Observations show galaxy mergers occur frequently in the universe, but so far no one has seen a merger of these giant black holes.

"We know galaxies with central combine all the time in the universe, yet we only see a small fraction of galaxies with two of them near their centers," said Scott Noble, an astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "The pairs we do see aren't emitting strong gravitational-wave signals because they're too far away from each other. Our goal is to identify—with alone—even closer pairs from which gravitational-wave signals may be detected in the future."

A paper describing the team's analysis of the new simulation was published Tuesday, Oct. 2, in the Astrophysical Journal and is now available online.

Scientists have detected merging stellar-mass black holes—which range from around three to several dozen solar masses—using the National Science Foundation's Laser Interferometer Gravitational-Wave Observatory (LIGO). Gravitational waves are space-time ripples traveling at the speed of light. They are created when massive orbiting objects like black holes and neutron stars spiral together and merge.

Gas glows brightly in this computer simulation of supermassive black holes only 40 orbits from merging. Models like this may eventually help scientists pinpoint real examples of these powerful binary systems. Credit: NASA's Goddard Space Flight Center

Supermassive mergers will be much more difficult to find than their stellar-mass cousins. One reason ground-based observatories can't detect gravitational waves from these events is because Earth itself is too noisy, shaking from seismic vibrations and gravitational changes from atmospheric disturbances. The detectors must be in space, like the Laser Interferometer Space Antenna (LISA) led by ESA (the European Space Agency) and planned for launch in the 2030s. Observatories monitoring sets of rapidly spinning, superdense stars called pulsars may detect gravitational waves from monster mergers. Like lighthouses, pulsars emit regularly timed beams of light that flash in and out of view as they rotate. Gravitational waves could cause slight changes in the timing of those flashes, but so far studies haven't yielded any detections.

But supermassive binaries nearing collision may have one thing stellar-mass binaries lack—a gas-rich environment. Scientists suspect the supernova explosion that creates a stellar black hole also blows away most of the surrounding gas. The black hole consumes what little remains so quickly there isn't much left to glow when the merger happens.

Supermassive binaries, on the other hand, result from galaxy mergers. Each supersized black hole brings along an entourage of gas and dust clouds, stars and planets. Scientists think a galaxy collision propels much of this material toward the central black holes, which consume it on a time scale similar to that needed for the binary to merge. As the black holes near, magnetic and gravitational forces heat the remaining gas, producing light astronomers should be able to see.

"It's very important to proceed on two tracks," said co-author Manuela Campanelli, director of the Center for Computational Relativity and Gravitation at the Rochester Institute of Technology in New York, who initiated this project nine years ago. "Modeling these events requires sophisticated computational tools that include all the physical effects produced by two supermassive black holes orbiting each other at a fraction of the speed of light. Knowing what light signals to expect from these events will help modern observations identify them. Modeling and observations will then feed into each other, helping us better understand what is happening at the hearts of most galaxies."

The new simulation shows three orbits of a pair of supermassive black holes only 40 orbits from merging. The models reveal the light emitted at this stage of the process may be dominated by UV light with some high-energy X-rays, similar to what's seen in any galaxy with a well-fed supermassive black hole.

This 360-degree video places the viewer in the middle of two circling supermassive black holes around 18.6 million miles (30 million kilometers) apart with an orbital period of 46 minutes. The simulation shows how the black holes distort the starry background and capture light, producing black hole silhouettes. A distinctive feature called a photon ring outlines the black holes. The entire system would have around 1 million times the Sun’s mass. Credit: NASA’s Goddard Space Flight Center; background, ESA/Gaia/DPAC

Three regions of light-emitting gas glow as the black holes merge, all connected by streams of hot gas: a large ring encircling the entire system, called the circumbinary disk, and two smaller ones around each black hole, called mini disks. All these objects emit predominantly UV light. When gas flows into a mini disk at a high rate, the disk's UV light interacts with each black hole's corona, a region of high-energy subatomic particles above and below the disk. This interaction produces X-rays. When the accretion rate is lower, UV light dims relative to the X-rays.

Based on the simulation, the researchers expect X-rays emitted by a near-merger will be brighter and more variable than X-rays seen from single supermassive black holes. The pace of the changes links to both the orbital speed of gas located at the inner edge of the circumbinary disk as well as that of the merging black holes.

"The way both black holes deflect light gives rise to complex lensing effects, as seen in the movie when one black hole passes in front of the other," said Stéphane d'Ascoli, a doctoral student at École Normale Supérieure in Paris and lead author of the paper. "Some exotic features came as a surprise, such as the eyebrow-shaped shadows one black hole occasionally creates near the horizon of the other."

The simulation ran on the National Center for Supercomputing Applications' Blue Waters supercomputer at the University of Illinois at Urbana-Champaign. Modeling three orbits of the system took 46 days on 9,600 computing cores. Campanelli said the collaboration was recently awarded additional time on Blue Waters to continue developing their models.

The original simulation estimated gas temperatures. The team plans to refine their code to model how changing parameters of the system, like temperature, distance, total mass and accretion rate, will affect the emitted light. They're interested in seeing what happens to gas traveling between the two black holes as well as modeling longer time spans.

"We need to find signals in the light from supermassive black hole binaries distinctive enough that astronomers can find these rare systems among the throng of bright single supermassive black holes," said co-author Julian Krolik, an astrophysicist at Johns Hopkins University in Baltimore. "If we can do that, we might be able to discover merging supermassive before they're seen by a space-based gravitational-wave observatory."

Explore further

Image: Black hole bounty captured in the center of the Milky Way

More information: Stéphane d'Ascoli et al. Electromagnetic Emission from Supermassive Binary Black Holes Approaching Merger, The Astrophysical Journal (2018). DOI: 10.3847/1538-4357/aad8b4
Journal information: Astrophysical Journal

Citation: New simulation sheds light on spiraling supermassive black holes (2018, October 2) retrieved 23 September 2019 from
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User comments

Oct 02, 2018
A caravan of dreamers, not BHs.

Oct 02, 2018
The Dance of the Leprechauns

Oct 03, 2018
^^^The mumbling of idiots.
Don't pay any attention to people who deny GR and all it's consequences. If you don't believe the theory and you don't believe the evidence, what have you got left?
Yes, posters like the above.

Note how they can never answer a direct question.
Note, when they do say something, it's mostly a rant devoid of content, as above.
Note when it does contain actual information, the argument presented will be based on a misunderstanding of said information.
Note, now they will disappear or the above will play out.
Note, they rarely disappear no matter how many times they are proven to be idiots that do not even understand the basics of what they are commenting on.
Note how they vote each other up even though they do not actually agree on anything, apart from "accepted science is WRONG".
Makes you wonder what they are doing on a science site, obviously can't be the science.
Must be the social interaction. What type of personality get a kick out of that?

Oct 03, 2018
I'm more interested in the region not modelled in the simulation...Why would they leave that out?

Oct 03, 2018
"Don't pay any attention to people who deny GR and all it's consequences. If you don't believe the theory and you don't believe the evidence, what have you got left?"

Likely an aversion to blind faith in what has become a patchwork quilt of invisible entities and fantastic claims as to what the entities do.

Note that every problem GR encounters is solved by inserting something that cannot be observed, experimented with, or actually proven to exist at all. Note that you cannot learn something from any simulation that has even one variable whose value is at best a guess because you are only learning something if the guess is correct. Note that the more we observe and the more math we do, the more we find observations which do not "fit" into GR, note that people who take a hard line stance on their beliefs and do not allow them to be malleable pending new observations wind up getting left behind and mothballed like the theories they refuse to see the problems with.

Oct 09, 2018
The most interesting part of the interaction is not simulated (the volume between the two masses). Is it feasible to fly a rocket ship vertically along the axis the two masses revolve about through this unsimulated space assuming that the black holes are supermassive to minimize spaghettification?

Theoretical method of forward time travel?

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