Gravity-censored fossil light
RESEARCHERS have discovered a subtle twist in the primeval light that formed shortly after the universe came into being. They hope it can reveal new secrets about the moments after the Big Bang.
This afterglow, called Cosmic Microwave Background, or CMB, was created out of hot ionized plasma some 13.7 billion years ago, when the universe was just 380,000 years old. A small fraction of this light is polarized (meaning the light waves vibrate in one plane).
Researchers had already detected this polarized light in one pattern, known as “electric” or E-mode polarization. But using the South Pole Telescope in Antarctica and the European Space Agency’s (ESA) Herschel space observatory, researchers for the first time detected polarized light from the CMB in the “magnetic” or B-mode.
The observed B-mode pattern arose from gravitational lensing, in which light gets bent and deflected by massive cosmic objects such as galaxy clusters and lumps of mysterious dark matter, researchers said.
But there is another way to produce B-modes as well: primordial gravitational waves produced during the earliest moments of the universe, when it was in its rapid “inflation” phase, mere trillionths of a second after the Big Bang.
During inflation, the idea goes, the universe expanded faster than thespeed of light, doubling in size 100 times or more in just a few tiny fractions of a second. (Einstein’s theory of special relativity holds that no information or matter can travel faster than light through space, but this rule does not apply to inflation, which was an expansion of space itself.)
The new detection should provide a sort of baseline that will aid future efforts to measure B-modes produced by gravitational waves, which in turn could reveal a great deal about how our universe grew in its earliest moments, researchers said.
Source: Live Science