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 on Sept. 14, 2015, at 4:51 a.m. CST by both of the twin Laser Interferometer Gravitational-wave Observatory, or LIGO, detectors, located in Livingston, La., and Hanford, Wash. The LIGO Observatories are funded by the National Science Foundation, or NSF, and were conceived, built and are operated by Caltech and MIT. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration, which includes the GEO Collaboration, the Australian Consortium for Interferometric Gravitational Astronomy and the Virgo Collaboration using data from the two LIGO detectors.
On Sept. 14, the LIGO instrument in Livingston, followed 7 milliseconds later by the instrument in Hanford, detected a gravitational wave signal from colliding black holes. The near simultaneous detection was necessary to confirm that the event was real, and indicated based on the relative time of arrival of the signals traveling at the speed of light, that the source was located in the southern hemisphere sky.
According to General Relativity, a pair of black holes orbiting around each other lose energy through the emission of gravitational waves, causing them to gradually approach each other over billions of years, and then much more quickly in the final minutes. During the final fraction of a second, the two black holes collide into each other at nearly one-half the speed of light and form a single more massive black hole, converting a portion of the combined black holes’ mass to energy according to Einstein’s formula E=mc2. This energy is emitted as a final strong burst of gravitational radiation.
Based on the physics of this particular event, LIGO scientists estimate that the two black holes in this event were about 29 and 36 times the mass of the sun, and that the event took place 1.3 billion years ago. About three times the mass of the sun was converted into gravitational waves in a fraction of a second—with a peak power output about 50 times that of the whole visible universe. LIGO observed these gravitational waves.
The LIGO Livingston observatory is located on LSU property, and LSU faculty, students and research staff are major contributors to the 15-nation international LIGO Science Collaboration, or LSC. More than 1,000 scientists from universities around the U.S. and 14 other countries conduct LIGO research as members of the LSC. More than 90 universities and research institutes in the LSC develop detector technology and analyze data; about 250 students are strong contributing members of the collaboration. 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, AEI), 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.
LSU’s investment in gravitational-wave detection spans more than four decades, and is among the longest of the institutions contributing to the present discovery. LSU faculty, students and scholars have had leading roles in the development of several generations of gravitational wave detectors, in their commissioning and operation as well as the collaborations formed. Today’s achievement is in part an outcome of LSU’s long-term vision and commitment to high-risk, high-potential gain scientific research.
Gabriela González, LSU professor of physics and astronomy, is the elected spokesperson, and leads the LSC. Together with other leaders and founders of the LIGO effort, González made the official statements and took questions starting on Thursday, Feb. 11, at the National Press Club in Washington, D.C., before gathered national science press. The announcement was also live streamed online.
“This detection is the beginning of a new era. The field of gravitational wave astronomy is now a reality,” González said.
Joseph Giaime, LSU professor of physics and astronomy, is the observatory head of LIGO Livingston.
“This first detection of gravitational waves owes its existence to the hard work over many years by hundreds of scientists, engineers and operations staff members. The breathtaking observation of a never-before-observed system of black holes had earned LIGO its `O’ as a completely new kind of astronomical observatory,” Giaime said.
LSU’s pioneering role in this science began in 1970 with the arrival of William Hamilton, now professor emeritus, who along with Physics Professor Warren Johnson, built and operated previous-generation cryogenic bar gravitational wave detectors on campus for many years. LSU Assistant Professor Thomas Corbitt focuses his research on advanced quantum metrology techniques for a future detector. This represents more than 45 years of cutting-edge research, with state and institutional commitment, and long-standing multimillion dollar support from NSF producing educational opportunities for students and postdoctoral researchers, several of whom have gone on to professorial appointments around the world.
LSU’s campus is located 25 miles from LIGO Livingston in Baton Rouge. LSU has about 1,600 faculty; 31,000 students; and is classified by the Carnegie Foundation as “Doctoral/Research Universities—Extensive.” LSU is the only research university in the U.S. located close enough for students and faculty to engage in daily interactions with a LIGO observatory. LSU faculty and administrators, including Chancellor Emeritus James Wharton, led the effort to bring LIGO to Louisiana, and the university owns the land on which LIGO is operated.
Both the Livingston and Hanford observatories function as L-shaped interferometers in which laser light is split into two beams that travel back and forth down 2.5 mile, or 4 kilometer, long arms that are 4 feet in diameter tubes kept under a near-perfect vacuum. The beams are used to monitor the distance between mirrors precisely positioned at the ends of the arms. According to Einstein’s theory, the distance between the mirrors will change by an infinitesimal amount when a gravitational wave passes by the detector. A change in the lengths of the arms smaller than one-ten-thousandth the diameter of a proton, or 10-19 meter, can be detected.
LIGO was originally proposed as a means of detecting gravitational waves in the 1980s by Rainer Weiss, professor of physics, emeritus, from MIT; Kip Thorne, Caltech’s Richard P. Feynman Professor of Theoretical Physics, emeritus; and Ronald Drever, professor of physics, emeritus, also from Caltech.
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, or CNRS, in France; eight from the Istituto Nazionale di Fisica Nucleare, or INFN, in Italy; two in The Netherlands with Nikhef; the Wigner RCP in Hungary; the POLGRAW group in Poland and the European Gravitational Observatory, or EGO, the laboratory hosting the Virgo detector near Pisa in Italy.
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. Advanced LIGO increased the volume of the universe probed and enabled the discovery of gravitational waves during its first observation run. NSF leads in financial support for Advanced LIGO. Funding organizations in Germany (Max Planck Society), the U.K. (Science and Technology Facilities Council, STFC) and Australia (Australian Research Council) also have made significant commitments to the project.
Several of the key technologies that made Advanced LIGO 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-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 the City of New York and LSU.
LIGO Livingston FAQ
What do we know about this first-ever detected gravitational wave?
LIGO has made the first-ever observations of gravitational waves arriving on Earth from space, and the first detection of two black holes colliding.
The gravitational wave signal was detected in Livingston and seven milliseconds later, the instrument at the LIGO observatory in Hanford, Washington detected the same gravitational wave. It confirms that black holes exist in binary systems with solar masses. It confirms aspects of Einstein’s Theory of General Relativity.]
From this, we will be able to learn more about gravity near a black hole, where space-time is warped, that would not be possible to learn in other ways.
How do the LIGO instruments work?
The LIGO detectors are interferometers that shine a laser through a vacuum down two arms in the shape of an L that are each 4 kilometers in length. The light from the laser bounces back and forth between mirrors on each end of the L. Scientists measure the length of both arms using the light.
If there’s a disturbance in space-time, such as a gravitational wave, the time the light takes to travel 4 kilometers will be slightly different in each arm making one arm look longer than the other. LIGO scientists measure the interference in the two beams of light when they come back to meet, which reveals information on the space-time disturbance.
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 observational run.
How do we know it’s a black hole?
The scientists compared the observation with Einstein’s prediction to identify that black holes produced this gravitational wave, how far they were, what the masses were and how large the final black hole was because of the energy emitted.
What is the LIGO Scientific Collaboration?
LIGO research is carried out by the LIGO Scientific Collaboration, or LSC, a group of more than1,000 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.
The LSC detector network includes the LIGO interferometers and the GEO600 detector. It includes matching LIGO facilities in Livingston, LA and Hanford, WA. The location of the two observatories with another one in Europe creates a triangle that can verify astronomical observations.
LSU Physics & Astronomy Professor Gabriela Gonzalez is the elected spokesperson for the LIGO Scientific Collaboration, a post she has held for five years. LSU Physics & AstronoProfessor Joe Giaime is the Observatory Head of LIGO Livingston.
What is LIGO Livingston?
LIGO Livingston is one of two laser interferometer observatories built to detect gravitational waves. About 40 people work at LIGO Livingston, which is about 36 miles north-east of Baton Rouge, Louisiana, where LSU is located. LIGO Livingston employs engineers, scientists and staff who support facilities, outreach and information technology to run the observatory. It is funded completely by the National Science Foundation, or NSF, and managed by the California Institute of Technology, or Caltech, and the Massachusetts Institute of Technology, or MIT. LSU owns the land, which is 180 acres, leased to the NSF until 2044.
LIGO Livingston began collecting data in 2005. In 2015, it received a major upgrade. The Advanced LIGO configurations increased the sensitivity of the instrumentation ten-fold. LIGO Livingston’s annual budget is $6-9 million per year.
About 17,000 people from the general public visit LIGO Livingston’s Science Education Center each year. Free hands-on educational activities are available for school groups as well as professional development training for educators.
This is only the beginning of the field of gravitational wave astronomy. LIGO Scientific Collaboration scientists continue to conduct research on the existing data and expect to detect more astronomical events as the LIGO detectors and technology become more sensitive, and the French-Italian gravitational wave detector, VIRGO, located in Cascina, Italy begins to collect data this year.
Scientists anticipate detecting other events including neutron stars in our galaxy, other black holes and supernova explosions.
At Long Last, Scientists Say They Have Confirmed Gravitational Waves
Gravitational waves: 'we can hear the universe'
Upgraded LIGO detectors spot gravitational waves
Einstein’s was right, gravitational waves do exist
Times of India
LIGO Hears Gravitational Waves, Einstein’s Universe ‘Speaking’
Einstein was right
Livingston LIGO lab helps detect Einstein-predicted space ripples
Gravitational waves detected 100 years after Einstein's prediction
National Science Foundation
Downloadable high-resolution images of LIGO Livingston: https://filestogeaux.lsu.edu/public/download.php?FILE=eperez2/27823SurZ91
LIGO Livingston video: https://youtu.be/6v_3JW9P9rk
LIGO website: https://ligo.caltech.edu/LA
NSF press conference archived video: https://www.youtube.com/watch?v=aEPIwEJmZyE
Observation of Gravitational Waves from a Binary Black Hole Merger, Physical Review Letters: http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.061102
Contact Ernie Ballard
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