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LIGO confirms RIT’s breakthrough prediction of gravitational waves


Research conducted by Rochester Institute of Technology scientists was integral to the breakthrough detection of gravitational waves from binary black holes that was announced today by the Laser Interferometer Gravitational-wave Observatory (LIGO) Scientific Collaboration.

The collaboration's findings confirm the existence of gravitational waves predicted by Albert Einstein's 1915 general theory of relativity and introduce a revolutionary new way of understanding the universe through gravitational wave astronomy. Six Rochester Institute of Technology researchers are among the authors on the upcoming paper in Physical Review Letters.

The LIGO paper prominently cites 2005 landmark research on binary black hole mergers led by Manuela Campanelli, director of RIT's Center for Computational Relativity and Gravitation. The signal detected by LIGO matches the numerical model of the waveform confirmed by RIT researchers and predicted in their 2005 breakthrough science, "Accurate Evolutions of Orbiting Black-Hole Binaries without Excision," originally published in Physical Review Letters, on March 22, 2006. The paper recently appeared in the American Physical Society's curated collection of seminal papers celebrating 100 years of Einstein's theory of general relativity.

Based on this milestone work from a decade ago, RIT researchers at the center, Carlos Lousto and James Healy, numerically modeled the merger of a pair of black holes and simulated gravitational waveforms. The actual wave patterns LIGO detected on Sept. 14, 2015, matched the simulations Lousto and Healy had created.

"The direct observation of a binary black hole merger by LIGO is an amazing confirmation of our theoretical calculations," said Campanelli, professor in RIT's School of Mathematical Sciences and an American Physical Society Fellow. "This is a historic moment in science."

The RIT team's breakthrough, known as the "moving puncture" approach, solved the interrelated equations for strong field gravity that comprise Einstein's theory of general relativity. Their method radically transformed the landscape of numerical relativity–a specialized field that solves Einstein's equations with sophisticated mathematics and supercomputers–and opened frontiers in gravitational wave astrophysics, Campanelli said.

RIT scientists used the moving puncture approach to make the first calculations of gravitational radiation from merging black holes with arbitrary masses and spins, and the discovery of large gravitational-radiation recoils from spinning supermassive black-hole mergers. The method also made possible their study of spin dynamics effects, such as spin-flips, precession and hang-up orbits, and extreme mass-ratio binaries.

"It is incredibly exciting to see the deep connections between theory and observation," said Lousto, a co-author on both the 2006 and LIGO breakthrough papers. "This is the Holy Grail of science. To confirm amazing predictions of general relativity is a dream come true. We have witnessed a historic event, the confirmation of the 100-year-old predictions of Einstein regarding gravitational waves and our 10-year-old computation of the merger of two black holes in a single event."

Collaborator Pedro Marronetti, program director of the division of gravitational physics at the National Science Foundation, noted that the simplicity and accuracy of their moving-puncture technique "opened up the field to a number of groups, large and small, all across the world."

RIT associate professor Yosef Zlochower, then a postdoctoral fellow and the fourth member of Campanelli's team, said, "We are witnessing the dawn of a new understanding of the universe," he said. "This has been decades in the making, and we are very proud to be part of this great effort."


For more information on the RIT team:

For information on CCRG: and

For information on RIT's Black Hole Lab:

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