Cosmologists at the Universities of Portsmouth and Rome, argue that the latest astronomical data favours a dark energy that grows as it interacts with dark matter, and this appears to be slowing the growth of structure in the cosmos.
"If the dark energy is growing and dark matter is evaporating we will end up with a big, empty, boring universe with almost nothing in it," said Professor David Wands, Director of Portsmouth's Institute of Cosmology and Gravitation.
Cosmology underwent a paradigm shift in 1998 when researchers announced that the rate at which the universe was expanding was accelerating, researchers said.
The idea of a constant dark energy throughout space-time (the "cosmological constant") became the standard model of cosmology, but now the Portsmouth and Rome researchers believe they have found a better description, including energy transfer between dark energy and dark matter.
"Much more data is available now than was available in 1998 and it appears that the standard model is no longer sufficient to describe all of the data. We think we've found a better model of dark energy," Wands said.
"Since the late 1990s astronomers have been convinced that something is causing the expansion of our universe to accelerate. The simplest explanation was that empty space - the vacuum - had an energy density that was a cosmological constant.
The findings appear in the journal Physical Review Letters, published by the American Physical Society.
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