On Tuesday the 3th of October, at least the several hundreds members of LIGO & VIRGO collaboration where anxiously waiting for the start of the streaming from the Swedish Academy of Science, around 11:30 CET, to follow the attribution of the Nobel Prize for Physics.
The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics 2017 with one half to
Rainer Weiss, LIGO/VIRGO Collaboration and the other half jointly to
Barry C. Barish, LIGO/VIRGO Collaboration and
Kip S. Thorne, LIGO/VIRGO Collaboration
“for decisive contributions to the LIGO detector and the observation of gravitational waves”
Cascina, 4 August 2017 – On Tuesday August 1st at 10 UCT the LIGO and VIRGO interferometers officially started taking data jointly.
Two perspectives justify the interest of international physics community on this date, the first concerns the conclusion of the construction and the start of operations of the European detector VIRGO, the second is the beginning of the systematic exploration of the Universe with the global network of new generation interferometers.
In September 2015, gravitational waves (GWs) were detected for the first time by the LIGO detectors, the two laser interferometers in the United States. It was found that detected GWs originate from the coalescence of two black holes (BHs) in a binary, each weighing about 30 times the mass of the Sun (30 solar mass). Although there have been indirect observations of BHs in the X-ray binaries, their masses are at most 15 solar masses.
With the announcement, on 11 February 2016, of the first detection ever of a gravitational wave by the LIGO and Virgo Collaborations, a New Astronomy, based on listening to the space-time vibrations, was born.
This long-awaited wave, 100 years after the theoretical prediction by Albert Einstein and 50 years after the first experimental efforts, arrived on Earth on 14 September 2015 and was finally perceived by humans with very smart “microphones”.