The direct detection of gravitational waves from at least five sources during the past two years offers spectacular confirmation of Einstein's model of gravity and space-time, researchers said.
Now, astronomers at Harvard-Smithsonian Center for Astrophysics (CfA) in the US have used a single gravitational wave event (GW170817) to measure the age of the universe.
A team of 1,314 scientists from around the world contributed to the detection of gravitational waves from a merging pair of binary neutron stars, followed by the detection of gamma-rays.
An analysis of the gravitational waves from this event infers their intrinsic strength.
The observed strength is less, implying that the source is about 140 million light-years away.
NGC4993, its host galaxy, has an outward velocity due to the expansion of the universe that can be measured from its spectral lines.
Knowing how far away it is and how fast the galaxy is moving from us allows scientists to calculate the time since the expansion began - the age of the universe: between about 11.9 and 15.7 billion years given the experimental uncertainties.
The former relies on mapping the very faint distribution of light dating from a time about four hundred thousand years after the big bang.
The latter involves a statistical analysis of the distances and motions of tens of thousands of galaxies in relatively recent times.
The fact that this one single gravitational-wave event was able to determine an age for the universe is remarkable, and not possible with every gravity wave detection.
With a large statistical sample of gravitational wave events of all types, the current range of values for the age will narrow, researchers said.
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