2014 March 18
Cosmic Microwave Map Swirls Indicate Inflation
Image Credit: BICEP2 Collaboration, NSF, Steffen Richter (Harvard)
Explanation: Did the universe undergo an early epoch of extremely rapid expansion? Such an
inflationary epoch has been postulated to explain several
puzzling cosmic attributes such as why our universe looks
similar in opposite directions. Yesterday,
results were released showing an expected signal of unexpected strength, bolstering a prediction of
inflation that specific patterns of
polarization should exist in
cosmic microwave background radiation -- light emitted 13.8 billion years ago as the
universe first became transparent. Called
B-mode polarizations, these early swirling patterns can be directly attributed to squeeze and stretch
effects that
gravitational radiation has on photon-emitting electrons. The
surprising results were
discovered in
data from the Background Imaging of Cosmic Extragalactic Polarization 2 (
BICEP2) microwave observatory near the South Pole.
BICEP2 is the building-mounted dish
pictured above on the left. Note how the black polarization vectors appear to swirl around the colored temperature peaks on the inset
microwave sky map. Although statistically
compelling, the conclusions will likely remain controversial while
confirmation attempts are made with independent observations.
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