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University of Mississippi

Gravitational Waves Detected 100 Years After Einstein’s Prediction

UM scientists join colleagues in celebration of historic achievement


Members of the UM LIGO Team include (from left) Camillo Cocchieri, visiting scholar; Mohammad Afrough, graduate student; Marco Cavaglia associate professor of of physics and astronomy; Katherine Dooley, assistant professor of physics and astronomy; and Jared Wofford and Hunter Gabbard, both undergraduate research assistants. Photo by Robert Jordan/Communications

Members of the UM LIGO Team include (from left) Camillo Cocchieri, visiting scholar; Mohammad Afrough, graduate student; Marco Cavaglia associate professor of of physics and astronomy; Katherine Dooley, assistant professor of physics and astronomy; and Jared Wofford and Hunter Gabbard, both undergraduate research assistants. Photo by Robert Jordan/Communications

For the first time, scientists have observed ripples in the fabric of space-time called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major prediction of Albert Einstein’s 1915 general theory of relativity and opens an unprecedented new window onto the cosmos.

Gravitational waves carry information about their dramatic origins and about the nature of gravity that cannot otherwise be obtained. Physicists have concluded that the detected gravitational waves were produced during the final fraction of a second of the merger of two black holes to produce a single, more massive spinning black hole. This collision of two black holes had been predicted but never observed.

The gravitational waves were detected at 4:51 a.m. Sept. 14, 2015 by both of the twin Laser Interferometer Gravitational-wave Observatory (LIGO) detectors in Livingston, Louisiana, and Hanford, Washington. The LIGO Observatories are funded by the National Science Foundation and were conceived, built and are operated by the California Institute of Technology and Massachusetts Institute of Technology.

The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration, which includes the GEO Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy, and the Virgo Collaboration using data from the two LIGO detectors.

“Using sophisticated algorithms and data analysis techniques, we estimate that the black hole collision took place about 1.3 billion years ago,” said Marco Cavaglià, University of Mississippi associate professor of physics and astronomy and assistant spokesperson of the LIGO Scientific Collaboration. “The two black holes had a mass of about 29 and 36 times the mass of the sun.”

The black holes collided with each other at nearly half the speed of light, said Katherine Dooley, UM assistant professor of physics and astronomy and senior member of the LIGO Scientific Collaboration.

“The explosion released so much energy that about three times the mass of the sun was converted to gravitational waves in only a fraction of a second,” Dooley said. “These are the gravitational waves that LIGO has observed.”

LIGO research is carried out by the LIGO Scientific Collaboration, a group of more than 1,000 scientists from universities around the United States and in 14 other countries. More than 90 universities and research institutes in the LSC develop detector technology and analyze data; approximately 250 students are strong contributing members of the collaboration.

UM has been a member of the LIGO Scientific Collaboration since 2007. Cavaglià founded the group at UM and has contributed to understanding artifacts of the instrument data that come from sources other than gravitational waves, a critical component for being able to positively identify a gravitational wave signal.

Since 2012, Cavaglià has served as the collaboration’s assistant spokesperson.

Dooley joined UM this past fall after having worked for over nine years on building and improving the LIGO and GEO600 detectors. The detectors use laser light to measure infinitesimal changes in the distance between mirrors mounted 2-1/2 miles (4 kilometers) apart.

“The detected gravitational waves changed this distance by one-billionth of a billionth of a meter, about one-thousandth the diameter of a proton,” Dooley said. She designed techniques to control the angular pointing of the laser beam, helping push the limits of the precision measurement technology that was needed to make this detection possible.

Cavaglià, Dooley, UM post-doctoral research assistant Shivaraj Kandhasamy and three doctoral students from the UM-LIGO team are among the authors of the discovery paper. The UM LIGO team also includes a master’s student, an undergraduate and three undergraduate exchange students from Italy.

“LIGO’s detection opens a new way to look at the cosmos,” Cavaglià said. “I think LIGO will go down in history in the same way as we now remember Galileo’s telescope.”

The entire university community shares in the excitement of this extraordinary achievement, UM Chancellor Jeffrey S. Vitter said.

“This astounding breakthrough is the result of decades of international collaboration by a talented team of scientists and engineers,” Vitter said. “Everyone at UM congratulates our colleagues in the physics department for their role in this historic discovery. The University of Mississippi is committed to pursuing research and scholarship that helps us understand and improve our world.”

The discovery was made possible by the enhanced capabilities of Advanced LIGO, a major upgrade that increases the sensitivity of the instruments, compared to the first-generation LIGO detectors, enabling a large increase in the volume of the universe probed – and the discovery of gravitational waves during its first observation run.

LIGO was originally proposed as a means of detecting these gravitational waves in the 1980s by Rainer Weiss, MIT professor emeritus of physics; Kip Thorne, Caltech’s Richard P. Feynman Professor Emeritus of Theoretical Physics; and Ronald Drever, Caltech professor emeritus of physics.

The LSC detector network includes the LIGO interferometers and the GEO600 detector. The GEO team includes scientists at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Leibniz Universität Hannover, along with partners at the University of Glasgow, Cardiff University, the University of Birmingham, other universities in the United Kingdom and the University of the Balearic Islands in Spain.

Several of the key technologies that made Advanced LIGO so much more sensitive have been developed and tested by the German UK GEO collaboration. Significant computer resources have been contributed by the AEI Hannover Atlas Cluster, the LIGO Laboratory, Syracuse University and the University of Wisconsin at Milwaukee.

Several universities designed, built and tested key components for Advanced LIGO: The Australian National University, the University of Adelaide, the University of Florida, Stanford University, Columbia University in New York and Louisiana State University.

The NSF leads in financial support for Advanced LIGO. Funding organizations in Germany (Max Planck Society), the U.K. (Science and Technology Facilities Council) and Australia (Australian Research Council) also have made significant commitments to the project.

Virgo research is carried out by the Virgo Collaboration, consisting of more than 250 physicists and engineers belonging to 19 different European research groups: six from Centre National de la Recherche Scientifique in France; eight from the Istituto Nazionale di Fisica Nucleare in Italy; two in The Netherlands with Nikhef; the Wigner RCP in Hungary; the POLGRAW group in Poland and the European Gravitational Observatory, the laboratory hosting the Virgo detector near Pisa in Italy.

“This is a momentous event,” Dooley said. “LIGO has opened our ears to the universe. For the first time ever, we can now listen to the cosmos.”

For more information on the UM LIGO team, go to