But they can still try and find evidence, and among the cosmologists searching for the weak signals which might remain will be John Carlstrom, the S. Chandrasekhar Distinguished Service Professor in Astronomy&Astrophysics at the University of Chicago. Carlstrom operates the South Pole Telescope (SPT) with a team of scientists from nine institutions in their search for evidence about the origins and evolution of the universe.
On their agenda is putting the cosmic inflation concept to an observational test: detecting extremely weak gravity waves, which Einstein's theory of general relativity predicts that cosmic inflation should produce.
"If you detect gravity waves, it tells you a whole lot about inflation for our universe," Carlstrom said. It also would rule out various competing ideas for the origin of the universe. "There are fewer than there used to be, but they don't predict that you have such an extreme, hot big bang, this quantum fluctuation, to start with," he said.
Nor would they produce gravity waves at detectable levels.
This simulation portrays the distortions in space and time at the subatomic scale, the result of quantum fluctuations occurring continuously throughout the universe. Near the end of the simulation, cosmic inflation begins to stretch space-time to the cosmic proportions of the universe. Source: Scott Dodelson, Fermilab/University of Chicago
"Since these are separate universes, by definition that means we can never have any contact with them. Nothing that happens there has any impact on us," said Scott Dodelson, a scientist at Fermi National Accelerator Laboratory and a Professor in Astronomy & Astrophysics at the University of Chicago.
But there is a way to probe the validity of cosmic inflation, they claim. The phenomenon would have produced two classes of perturbations. The first, fluctuations in the density of subatomic particles happen continuously throughout the universe, and scientists have already observed them.
"Usually they're just taking place on the atomic scale. We never even notice them," Dodelson said. But inflation would instantaneously stretch these perturbations into cosmic proportions. "That picture actually works. We can calculate what those perturbations should look like, and it turns out they are exactly right to produce the galaxies we see in the universe."
The second class of perturbations would be gravity waves—Einsteinian distortions in space and time. Gravity waves also would get promoted to cosmic proportions, perhaps even strong enough for cosmologists to detect them with sensitive telescopes tuned to the proper frequency of electromagnetic radiation.
The aurora australis (southern lights) over the South Pole Telescope. Photo: Keith Vanderlinde
"We should be able to see them if John's instruments are sensitive enough," Dodelson said.
The group is building a special instrument, a polarimeter, as an attachment to the SPT, to search for gravity waves. The SPT operates at submillimeter wavelengths, between microwaves and the infrared on the electromagnetic spectrum.
Cosmologists also use the SPT in their quest to solve the mystery of 'dark energy'. A hypothetical repulsive force, dark energy pushes the universe apart and overwhelms gravity, the attractive force exerted by all matter. Dark energy is invisible, but astronomers believe it exists because they would explain the effects on clusters of galaxies that formed within the last few billion years.
The SPT detects the cosmic microwave background (CMB) radiation, the afterglow of the big bang. Cosmologists have mined a fortune of data from the CMB, which represent the forceful drums and horns of the cosmic symphony. But now the scientific community has its ears cocked for the tones of a subtler instrument—gravitational waves—that underlay the CMB.
"We have these key components to our picture of the universe, but we really don't know what physics produces any of them," said Dodelson of inflation, dark energy and the equally mysterious dark matter. "The goal of the next decade is to identify the physics."
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