A trio of U.S. scientists received the 2017 Nobel Prize in Physics on Tuesday for their role in the study of gravitational waves – and their colleagues at Syracuse University are applauding the achievement.
The 2017 Nobel Prize in Physics was awarded to Rainer Weiss, Barry C. Barish and Kip S. Thorne for their detection of gravitational waves, a development scientists believe could give vital clues to the origins of the universe.
SU boasts several faculty members who were involved in the discovery of gravitational waves using LIGO – Duncan Brown, Peter Saulson, and Stefan Ballmer.
“We always knew how cool it would be to make that first detection. But I don’t think that any of us realized how strongly it would capture the imagination of people around the world. That has been tremendously gratifying,” Saulson said.
Weiss hired Saulson for his first job as a physicist, giving him a chance to help design the Laser Interferometer Gravitational-Wave Observatory.
“Rai took a chance on me and gave me the opportunity to contribute to something marvelous. And it’s not just me; the LIGO team is filled with people who revere Rai as a model physicist and a caring human being,” Saulson said.
On Tuesday, they were reflecting on their achievement, and celebrating the Weiss, Barish, and Thorne’s acceptance of the prestigious award.
“They are true visionaries and whose leadership has created the new field of gravitational-wave astronomy. They have also been kind and patient mentors to many generations of scientists, including Stefan, Peter, and me,” Brown said.
Gravitational waves are “ripples” in the fabric of space and time caused by some of the most violent and energetic processes in the universe, according to the California Institute of Technology (Caltech).
The strongest gravitational waves are produced by catastrophic events, such as colliding black holes, and the LIGO detector is essentially a “black hole telescope,” allowing scientists to “see” what was previously invisible.
“On 14 September 2015, the universe’s gravitational waves were observed for the very first time,” the Nobel committee wrote in a press release.
“The waves, which were predicted by Albert Einstein a hundred years ago, came from a collision between two black holes. It took 1.3 billion years for the waves to arrive at the LIGO detector in the USA.
“The signal was extremely weak when it reached Earth, but is already promising a revolution in astrophysics,” the committee added.
“Gravitational waves are an entirely new way of observing the most violent events in space and testing the limits of our knowledge.”
‘Look deeper into the universe’
The award was given half to Weiss from the Massachusetts Institute of Technology and the other half jointly to Barish and Thorne from Caltech.
Around 1,000 people have worked on the development of the technology over four decades, according to Weiss and the Nobel committee.
“(They are) people who have been thinking about this, sometimes failing and slowly getting the technology together to do this — it’s exciting that they’re finally doing this,” Weiss said, speaking at the conference by phone.
He said that as the detectors develop and become more sensitive, scientists will be able to look deeper into the universe and gain more insights into the origins of the universe.
“We fully expect to learn about things we didn’t know about, not just black holes.”
Professor Sheila Rowan, Director of the University of Glasgow’s Institute for Gravitational Research, was one of the UK’s leads on LIGO and welcomed the Nobel committee’s decision.
“The discovery of the existence of gravitational waves, just over two years ago, has opened up a whole new way to understand the universe,” she said.
Each of the six Nobel prizes come with an award of 9 million Swedish kronor ($1.1 million), which is shared when there are multiple recipients.
Alfred Nobel created five prizes in his 1895 will for medicine, physics, chemistry, literature and peace. A sixth prize in economics was created, in Nobel’s memory, by Sweden’s central bank in 1968.
For more information on LIGO, click here.