Ripples in the universe from the Big Bang

A team of US astronomers, after years of working in the Antarctic, say they have found long-awaited evidence for the theory that the Universe underwent a period of rapid “inflation” in the very first moments of its existence. They also provide the most direct evidence for the existence of gravitational waves, and thus gravitons, which were predicted by Albert Einstein almost a century ago.

Proof of cosmic inflation

In 1979, cosmologist Professor Alan Guth, then a young physicist at Stanford University, had theorised that immediately following the moment of the Big Bang the Universe underwent a process of inflation – an ultra-rapid expansion that took it from subatomic size to a scale so vast that the human mind can barely conceive the distances involved almost instantaneously. Although widely accepted, for three decades the theory has lacked proof, it was fitting then that the principal investigator of the team, astronomer Professor John Kovac from the Harvard-Smithsonian Center for Astrophysics, would visit Professor Alan Guth as one of the first people outside of the research team to be informed that proof was finally at hand before the news went public.

Professor Kovac led a team of radio astronomers who have been monitoring the skies over the South Pole since 2010 using an ultra-sensitive microwave receiver known as BICEP2.

They were able to detect subtle patterns, a type of light polarization called "B-modes", in the cosmic microwave background – the afterglow of the Big Bang which saturates the universe, which they believe could only be caused by the gravitational waves predicted by Einstein. The waves also provide proof of Professor Guth’s theory of cosmic inflation, and apparently open “a window into the unification of the fundamental forces of nature”.

The existence of gravitons

In an interview with Mike Wall, a Senior Writer at space.com , Professor Kovac said an implication of “seeing gravitational waves at the strength that we've seen them is that, yes, in fact, that is the energy scale of inflation. And another thing that is an important aspect of this that is quite fundamental is that the production of these gravitational waves during the inflationary process relies on the interaction of quantum mechanics and general relativity. It actually relies on there being gravitons, the gravitational field being quantized. And that is something of which we'd had no prior direct evidence.”

B-modes the “smoking gun”

In an interview with the Science Media Centre, Professor Richard Easther, HOD of physics at the University of Auckland, said, "The word is that the BICEP team has discovered B-modes, specific patterns in the polarisation of the microwave background. B-modes are the "smoking gun" of inflation, and their strength is tied to the energy density of the universe during inflation - if the rumours hold up, we could soon know that inflation did happen a trillion, trillion, trillionth of a second after the Big Bang, and at energies a trillion times beyond the reach of the Large Hadron Collider.

"There would still be several steps to nailing it down - not all B-mode signals must come from inflation, and not all inflationary models must produce detectable B-modes. And there's one more thing: the B-mode is sourced by gravitational waves - ripples in the fabric of space - generated during inflation.

"Gravitational waves are a key prediction of Einstein's General Relativity and their existence is still not conclusively confirmed. Even so, gravitational waves are getting second billing to what we will learn about the early universe: we will know that inflation is a compelling answer to cosmology's initial-conditions problems, and humankind will have looked directly into the cosmic dawn.”

After painstakingly checking and rechecking their measurements, the US team made the results public on 17 March 2014 at a press conference at the Harvard-Smithsonian Centre for Astrophysics.

The discovery, if confirmed by other teams of astronomers, is widely-tipped to be worthy of a Nobel Prize. At the very least, being able to observe the signature of gravitational waves from the Big Bang will open a new chapter in astronomy, cosmology and physics.