Interpreting Asymmetry In Early Universe
The Big Bang is widely considered to have obliterated any trace of what came before. Now, astrophysicists at the California Institute of Technology (Caltech) think that their new theoretical interpretation of an imprint from the earliest stages of the universe may also shed light on what came before.
“It’s no longer completely crazy to ask what happened before the Big Bang,” comments Marc Kamionkowski, Caltech’s Robinson Professor of Theoretical Physics and Astrophysics. Kamionkowski joined graduate student Adrienne Erickcek and senior research associate in physics Sean Carroll to propose a mathematical model explaining an anomaly in what is supposed to be a universe of uniformly distributed radiation and matter.
Their investigations turn on a phenomenon called inflation, first proposed in 1980, which posits that space expanded exponentially in the instant following the Big Bang. “Inflation starts the universe with a blank slate,” Erickcek describes. The hiccup in inflation, however, is that the universe is not as uniform as the simplest form of the theory predicts it to be. Some parts of it are more intensely varied than others.
Until recently, measurements of the Cosmic Microwave Background (CMB) radiation, a form of electromagnetic radiation that permeated the universe 400,000 years after the Big Bang, were consistent with inflation–miniscule fluctuations in the CMB seemed to be the same everywhere. But a few years ago, some researchers, including a group led by Krzysztof Gorski of NASA’s Jet Propulsion Laboratory, which is managed by Caltech, scrutinized data from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP). They discovered that the amplitude of fluctuations in the CMB is not the same in all directions.
“If your eyes measured radio frequency, you’d see the entire sky glowing. This is what WMAP sees,” Kamionkowksi describes. WMAP depicts the CMB as an afterglow of light from shortly after the Big Bang that has decayed to microwave radiation as the universe expanded over the past 13.7 billion years. The probe also reveals more pronounced mottling–deviations from the average value–in the CMB in one half of the sky than the other.
“It’s a certified anomaly,” Kamionkowski remarks. “But since inflation seems to do so well with everything else, it seems premature to discard the theory.” Instead, the team worked with the theory in their math addressing the asymmetry.
They started by testing whether the value of a single energy field thought to have driven inflation, called the inflaton, was different on one side of the universe than the other. It didn’t work–they found that if they changed the mean value of the inflaton, then the mean temperature and amplitude of energy variations in space also changed. So they explored a second energy field, called the curvaton, which had been previously proposed to give rise to the fluctuations observed in the CMB. They introduced a perturbation to the curvaton field that turns out to affect only how temperature varies from point to point through space, while preserving its average value.
The new model predicts more cold than hot spots in the CMB, Kamionkowski says. Erickcek adds that this prediction will be tested by the Planck satellite, an international mission led by the European Space Agency with significant contributions from NASA, scheduled to launch in April 2009.
For Erickcek, the team’s findings hold the key to understanding more about inflation. “Inflation is a description of how the universe expanded,” she adds. “Its predictions have been verified, but what drove it and how long did it last? This is a way to look at what happened during inflation, which has a lot of blanks waiting to be filled in.”
But the perturbation that the researchers introduced may also offer the first glimpse at what came before the Big Bang, because it could be an imprint inherited from the time before inflation. “All of that stuff is hidden by a veil, observationally,” Kamionkowski says. “If our model holds up, we may have a chance to see beyond this veil.”
The study appears December 16 in the journal Physical Review D. It was supported by the Department of Energy and by Caltech’s Moore Center for Theoretical Cosmology and Physics.
Image Caption: This is the cosmic microwave background as seen by the WMAP satellite. This radiation was emitted when the Universe was 380,000 years old and has an average temperature of 2.7 Kelvin. The red and blue spots are temperature fluctuations that differ from the average temperature by only 0.0002 degrees. The region of maximal variation is in the lower right quadrant. Credit: NASA/WMAP Science Team
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