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ASTRONOMY Nobel awarded for gravitational-wave detection , and share the prize for their work at LIGO.

BY DAVIDE CASTELVECCHI

hree who had leading roles in the first direct detection of gravita- tional waves have won the 2017 Nobel TPrize in Physics. Rainer Weiss, at the Mas- sachusetts Institute of Technology (MIT) in Cambridge, and Barry Barish and Kip Thorne, both at the California Institute of Technology in Pasadena, share the 9-million-Swedish-krona (US$1.1-million) award for their work at the US-based Interferometer Gravitational- Wave Observatory (LIGO). In September 2015, LIGO picked up the deformations in -time caused by the collision of distant black holes. That discovery, which was announced in February 2016, opened up a new of astron- omy, in which scientists listen to the space-time Catching waves (from left): Barry Barish, Rainer Weiss and Kip Thorne.

LEFT: CALTECH; CENTRE: BRYCE VICKMARK/MIT; RIGHT: CALTECH ALUMNI ASSOC. ALUMNI CALTECH RIGHT: VICKMARK/MIT; CENTRE: BRYCE CALTECH; LEFT: vibrations emitted by some of the ’s most cataclysmic events. And it confirmed the deformations — those produced by collapsing not fund two separate efforts, and the LIGO col- existence of gravitational waves, which Albert stars or colliding black holes — would typically laboration was born. Einstein had predicted a century before. be tiny by the time they reached Earth. The The troika did not always work smoothly and, Weiss and Thorne are two of three physicists waves detected in 2015 stretched and squeezed at its members’ own admission, did not have known as the troika — the founders of LIGO’s LIGO’s perpendicular 4-kilometre vacuum the right skills for managing what was quickly giant twin detectors in Livingston, , pipes by a fraction of a ’s width, but that becoming a vast operation. Things improved and in Hanford, . The third troika was enough to noticeably shift out of sync the dramatically after Barish, who had been LIGO’s member, , died on 7 March this laser beams bouncing inside the pipes. principal investigator since 1994, became direc- year. Barish, who was LIGO director from 1997 Physicists in the United States and the then- tor in 1997. “Without Barish turning things to 2005, is widely credited with transforming Soviet Union first proposed using laser inter- around, it would have collapsed,” says Collins. the collaboration from a chaotic endeavour to ferometers to detect gravitational waves in the LIGO ended up being the largest and most a well-oiled machine. 1960s. Weiss made the first detailed calcula- expensive experiment in the history of the US “I view this more as a thing that recognizes tions for how an interferometer would work National Science Foundation. Its two detectors the work of about 1,000 people, a really dedi- in 1972. The idea seemed so far-fetched that first opened in 2002, with an admittedly scant cated effort that’s been going on for — I hate even he was not sure it would work. “It might chance of finding anything during their first to tell you — as long as 40 years,” said Weiss in come to a junction in a year or so when we will phase of data collection. The observatory shut an interview with the Nobel Committee. He is decide it ain’t worth it,” he told science soci- down in 2010 for an overhaul and restarted in awarded half the prize, with the other half split ologist Harry Collins at the time (H. Collins September 2015, three times more sensitive between Barish and Thorne. ’s Shadow; Univ. Chicago Press, 2004). than before. The Universe was kind to LIGO, Weiss, who was born in Germany in 1932, providing a dramatic for it to record on UNIMPEDED MOTION emigrated with his family to the United States 14 September while the interferometers were Few physicists doubted the existence of gravi- in 1938 to escape from . He built his first still being calibrated, days before their official tational waves before LIGO’s discovery. These prototype interferometer in the mid-1970s, fol- science run was due to start. Since then, LIGO distortions in space-time are a consequence of lowed by researchers in Europe — among them, has detected at least three other gravitational- Einstein’s general , and prop- Drever and his collaborators at the University of wave events — the most recently reported with agate across the Universe almost unimpeded. Glasgow, UK. Virgo, a similar interferometer near Pisa, . In 1974, they were confirmed indirectly when Thorne specialized in and Thorne and Weiss were generally considered researchers examined the radio flashes emitted had also been developing ideas on the waves. At shoo-ins for the Nobel. Before Drever’s pass- by a pair of merging neutron stars; the shifts in a conference in Washington DC in 1975, he and ing in March, the troika racked up almost the flashes’ timing matched predictions of how Weiss shared a room in an over-booked hotel. every prize there was to win, including the gravitational waves would carry away During their conversations, Weiss convinced $3-million Special in from the event. That discovery was rewarded Thorne that interferometers were the right Fundamental Physics; the $500,000 Gruber with the 1993 in Physics. approach. Thorne, Weiss and Drever joined Foundation Cosmology Prize; the $1.2-million But sensing the waves themselves was a forces in the early 1980s, when it became clear in ; and the $1-million monumental task. Even the most powerful that the US National Science Foundation would in . ■

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