Scientists are claiming a stunning discovery in their quest to fully understand gravity.
They have observed the warping of space-time generated by the collision of two black holes more than a billion light-years from Earth.
The international team says the first detection of these gravitational waves will usher in a new era for astronomy.
It is the culmination of decades of searching and could ultimately offer a window on the Big Bang.
The research, by the Ligo Collaboration, has been accepted for publication in the journal Physical Review Letters.
The collaboration operates a number of labs around the world that fire lasers through long tunnels, trying to sense ripples in the fabric of space-time.
Expected signals are extremely subtle, and disturb the machines, known as interferometers, by just fractions of the width of an atom.
But the black hole merger was picked up by two widely separated LIGO facilities in the US.
“We have detected gravitational waves,” David Reitze, executive director of the Ligo project, told journalists at a news conference in Washington DC.
Prof Karsten Danzmann, from the Max Planck Institute for Gravitational Physics and Leibniz University in Hannover, Germany, is a European leader on the collaboration.
He said the detection was one of the most important developments in science since the discovery of the Higgs particle, and on a par with the determination of the structure of DNA.
“There is a Nobel Prize in it – there is no doubt,” he told the BBC.
“It is the first ever direct detection of gravitational waves; it’s the first ever direct detection of black holes and it is a confirmation of General Relativity because the property of these black holes agrees exactly with what Einstein predicted almost exactly 100 years ago.”
Ripples in the fabric of space-time
- Gravitational waves are prediction of the Theory of General Relativity
- Their existence has been inferred by science but only now directly detected
- They are ripples in the fabric of space and time produced by violent events
- Accelerating masses will produce waves that propagate at the speed of light
- Detectable sources ought to include merging black holes and neutron stars
- LIGO fires lasers into long, L-shaped tunnels; the waves disturb the light
- Detecting the waves opens up the Universe to completely new investigations
That view was reinforced by Professor Stephen Hawking, who is an expert on black holes. Speaking exclusively to BBC News he said he believed that the detection marked a moment in scientific history.
“Gravitational waves provide a completely new way at looking at the Universe. The ability to detect them has the potential to revolutionise astronomy. This discovery is the first detection of a black hole binary system and the first observation of black holes merging,” he said.
“Apart from testing (Albert Einstein’s theory of) General Relativity, we could hope to see black holes through the history of the Universe. We may even see relics of the very early Universe during the Big Bang at some of the most extreme energies possible.”
The Ligo laser interferometers in Hanford, in Washington, and Livingstone, in Louisiana, were only recently refurbished and had just come back online when they sensed the signal from the collision. This occurred at 10.51 GMT on 14 September last year.
On a graph, the data looks like a symmetrical, wiggly line that gradually increases in height and then suddenly fades away.
“We found a beautiful signature from of the merger of two black holes and it agrees exactly – fantastically – with the numerical solutions to Einstein equations… it looked too beautiful to be true,” said Prof Danzmann.
Prof Sheila Rowan, who is one of the lead UK researchers involved in the project, said that the first detection of gravitational waves was just the start of a “terrifically exciting” journey.
“The fact that we are sitting here on Earth feeling the actual fabric of the Universe stretch and compress slightly due to the merger of black holes that occurred just over a billion years ago – I think that’s phenomenal. It’s amazing that when we first turned on our detectors, the Universe was ready and waiting to say ‘hello’,” the Glasgow University scientist told the BBC.
Being able to detect gravitational waves enables astronomers finally to probe what they call “dark Universe” – the majority part of the cosmos that is invisible to the light telescopes in use today.
Perfect probe
Not only will they be able to investigate black holes and strange objects known as neutron stars (giant suns that have collapsed to the size of cities), they should also be able to “look” much deeper into the Universe – and thus farther back in time. It may even be possible eventually to sense the moment of the Big Bang.
“Gravitational waves go through everything. They are hardly affected by what they pass through, and that means that they are perfect messengers,” said Prof Bernard Schutz, from Cardiff University, UK.
“The information carried on the gravitational wave is exactly the same as when the system sent it out; and that is unusual in astronomy. We can’t see light from whole regions of our own galaxy because of the dust that is in the way, and we can’t see the early part of the Big Bang because the Universe was opaque to light earlier than a certain time.
“With gravitational waves, we do expect eventually to see the Big Bang itself,” he told the BBC.
In addition, the study of gravitational waves may ultimately help scientists in their quest to solve some of the biggest problems in physics, such as the unification of forces, linking quantum theory with gravity.
At the moment, the General Relativity describes the cosmos on the largest scales tremendously well, but it is to quantum ideas that we resort when talking about the smallest interactions. Being able to study places in the Universe where gravity is extreme, such as at black holes, may open a path to new, more complete thinking on these issues.
- A laser is fed into the machine and its beam is split along two paths
- The separate paths bounce back and forth between damped mirrors
- Eventually, the two light parts are recombined and sent to a detector
- Gravitational waves passing through the lab should disturb the set-up
- Theory holds they should very subtly stretch and squeeze its space
- This ought to show itself as a change in the lengths of the light arms (green)
- The photodetector captures this signal in the recombined beam
Scientists have sought experimental evidence for gravitational waves for more than 40 years.
Einstein himself actually thought a detection might be beyond the reach of technology.
His theory of General Relativity suggests that objects such as stars and planets can warp space around them – in the same way that a billiard ball creates a dip when placed on a thin, stretched, rubber sheet.
Gravity is a consequence of that distortion – objects will be attracted to the warped space in the same way that a pea will fall in to the dip created by the billiard ball.
Inspirational moment
Einstein predicted that if the gravity in an area was changed suddenly – by an exploding star, say – waves of gravitational energy would ripple across the Universe at light-speed, stretching and squeezing space as they travelled.
Although a fantastically small effect, modern technology has now risen to the challenge.
Much of the R&D work for the Washington and Louisiana machines was done at Europe’s smaller GEO600 interferometer in Hannover.
“I think it’s phenomenal to be able to build an instrument capable of measuring [gravitational waves],” said Prof Rowan.
“It is hugely exciting for a whole generation of young people coming along, because these kinds of observations and this real pushing back of the frontiers is really what inspires a lot of young people to get into science and engineering.”
