New Type of Dark Energy Could Solve Universe Expansion Mystery

Cosmologists have found signs that a second type of dark energy -- the ubiquitous but enigmatic substance that is pushing the current Universe's expansion to accelerate -- might have existed in the first 300,000 years after the Big Bang. From a report: Two separate studies -- both posted on the arXiv preprint server in the past week -- have detected a tentative first trace of this 'early dark energy' in data collected between 2013 and 2016 by the Atacama Cosmology Telescope (ACT) in Chile. If the findings are confirmed, they could help to solve a long-standing conundrum surrounding data about the early Universe, which seem to be incompatible with the rate of cosmic expansion measured today. But the data are preliminary and don't show definitively whether this form of dark energy really existed.

'There are a number of reasons to be careful to take this as a discovery of new physics,' says Silvia Galli, a cosmologist at the Paris Institute of Astrophysics. The authors of both preprints -- one posted by the ACT team, and the other by an independent group -- admit that the data are not yet strong enough to detect early dark energy with high confidence. But they say that further observations from the ACT and another observatory, the South Pole Telescope in Antarctica, could provide a more stringent test soon. 'If this really is true -- if the early Universe really did feature early dark energy -- then we should see a strong signal,' says Colin Hill, a co-author of the ACT team's paper who is a cosmologist at Columbia University in New York City.

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