Scientists Use Light Signatures to Track Merging Supermassive Black Holes

RIT and Johns Hopkins University collaborate on $2M project

A. Sue Weisler

Using computer models, astrophysicists from Rochester Institute of Technology and Johns Hopkins University are tracing electromagnetic signatures from black hole collisions. The team, led by Manuela Campanelli, director of the Center for Computational Relativity and Gravitation at RIT, has won a $2 million grant from the National Science Foundation.

Scientists pursuing supermassive black holes suspect that these giants merge somewhere in the universe roughly once a year, but they don’t know how to find them. They think the evidence is hidden in the powerful gravitational waves and strong bursts of electromagnetic radiation created when the black holes collide.

Using computer models, astrophysicists from Rochester Institute of Technology and Johns Hopkins University are tracing electromagnetic signatures back to the impact. They are creating a detailed blueprint that will guide other scientists searching for merging black holes using ordinary visible light and existing telescopes. Simulated models of these mergers will also aid the discovery of gravitational waves, proving Einstein’s theory of general relativity.

The team, led by Manuela Campanelli, director of the Center for Computational Relativity and Gravitation at RIT, has won a $2 million grant from the cyber-enabled discovery and innovation program of the National Science Foundation. Julian Krolik is leading the collaboration’s efforts at Johns Hopkins, where he is a professor in the Department of Physics and Astronomy. Both institutions received $1 million awards for the five-year project.

The scientists will use computer models to simulate what happens to an accretion disk—a doughnut-shaped ring of gas and dust—as a pair of black holes within it approach each other and merge. According to Campanelli, the surrounding gas and dust mixture is heated and will likely produce electromagnetic radiation—light—that could be detected by conventional telescopes, such as the Large Synoptic Survey Telescope, even before sufficiently sensitive gravitational wave telescopes are built.

“By being able to model this for the first time in a realistic scenario, with realistic conditions, we should be able to predict signals of binary black hole mergers that can be seen in the electromagnetic sky,” says Campanelli, associate professor in the School of Mathematical Sciences at RIT. “It’s a big deal because nobody has ever attempted a consistent and long-term project to model such a phenomenon.”

“The goal is to get a very accurate and consistent model of the electromagnetic emission from something that is also emitting strong gravitational waves,” adds Scott Noble, associate research scientist in the Center for Computational Relativity and Gravitation. “And I think the significance of the project is that we’re doing this in a very careful, methodical way.”

Yosef Zlochower, an assistant professor in the School of Mathematical Sciences and research faculty in the center, says, “Our project will make use of combined expertise in the simulation of generic black-hole binaries with magneto-hydrodynamics simulations to model the accretion disk physics during the last phases of the binary, when both space and time are very dynamical.”

No easy feat, the problem requires solving the equations describing the behavior of ionized gases threaded by magnetic fields along with the equations comprising Einstein’s theory of general relativity, Campanelli explains. Looking at binary black hole mergers through complementary signals—gravitational waves and electromagnetic waves—introduces a new type of astronomy.

“From the electromagnetic radiation, you can clearly determine direction,” Campanelli says. “We’d be able to connect a lot of the physics happening within the gaseous environment and accretion disk to the binary black hole merger to the gravitational radiation. It will be multi-messenger astronomy because it’s electromagnetic combined with gravitational radiation.”

Krolik’s team at Johns Hopkins will model the premerger stage of the binary black holes using Newton’s law of gravity to describe masses that are far apart. Campanelli’s group at RIT will look at what happens when Newtonian physics breaks down and the black holes draw closer together and actually merge. Both teams will address the post-merger physics.

“We want to marry the two regimes and use the far-field results to feed into the close-field results to get a consistent picture of how these systems evolved in time,” Noble says.

The multilayered problem describes various stages of the merger in gaseous environments. Both teams are trying to “connect the dots” in this massive problem that draws on gravitational radiation and magneto-hydrodynamics, the theory that governs the dynamics of gas or plasma in strongly gravitating systems.

The project brings together leaders in black hole research. Campanelli and team members Carlos Lousto and Zlochower announced a numerical breakthrough in 2005 that, for the first time, enabled calculation of how black holes merge, a task requiring large supercomputers. Krolik is known for his work on active galactic nuclei (single, very large black holes at the centers of galaxies that rapidly swallow surrounding gas), and is a leading expert in magneto-hydrodynamic theory, along with contributing scientists Jim Stone of Princeton University and John Hawley of the University of Virginia.

“The effort is therefore strongly multidisciplinary because of the multiple kinds of expertise needed: numerical relativity, magneto-hydrodynamical simulation, advanced computational techniques, including parallel computing, the use of very large data sets, scientific visualization and observational astronomy,” Campanelli says.

“It’s a very challenging computational problem,” she adds. “It’s huge. If you think of how complicated these black hole coalescences are without any gas or electric fields, you can imagine—when you add electromagnetic radiation and gas—that we will have very demanding simulations.”

Simulating the merger of binary black holes in gaseous environments requires access to considerable computer power. The RIT team will run the actual merger on its own computer, NewHorizons, and make use of additional resources.

“The project will generate a much larger amount of data than we are currently generating,” says Lousto, associate professor in the School of Mathematical Sciences at RIT. “Money allocated in the grant will add 200 terabytes of storage and processing power to the center’s computer.”

The RIT-Johns Hopkins team will also make use of other resources such as the machine known as Blue Waters at the University of Illinois’ National Center for Supercomputing Applications.

The RIT team will also work closely with mathematics professors and Joshua Faber and John Whelan; postdoctoral researchers Hiroyuki Nakano and Bruno Mundim; and astrophysical sciences and technology graduate students Marcelo Ponce, Billy Vazquez, Prabath Peires and Ian Ruchlin. The scientific visualizations will be done in collaboration with Hans-Peter Bischof, graduate coordinator in the computer science department in the B. Thomas Golisano College of Computing and Information Sciences and member of the doctoral program in Computing and Information Sciences.


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