Durham astronomers’ doubts about the “Dark Side”
(16 June 2010)
New research by astronomers at Durham University suggests conventional wisdom about the content of the Universe may be wrong.
Graduate student Utane Sawangwit and Professor Tom Shanks, in Durham's Department of Physics, looked at observations from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite to study the remnant heat from the Big Bang.
The two scientists found evidence that the errors in its data may be much larger than previously thought, which in turn makes the standard model of the Universe open to question.
They published their results in a letter to the journal Monthly Notices of the Royal Astronomical Society.
Launched in 2001, WMAP measures differences in Cosmic Microwave Background (CMB) radiation, the residual heat of the Big Bang that fills the Universe and appears over the whole of the sky.
The angular size of the ripples in the CMB is thought to be connected to the composition of the Universe. The observations of WMAP showed that the ripples were about twice the size of the full Moon, or around a degree across.
With these results, scientists concluded that the cosmos was made up of four per cent 'normal' matter, 22 per cent 'dark' or invisible matter and 74 per cent 'dark energy'. Debate about the exact nature of the 'dark side' of the Universe - the dark matter and dark energy - continues to this day.
Sawangwit and Shanks used astronomical objects that appear as unresolved points in radio telescopes to test the way the WMAP telescope smoothes out its maps. They found that the smoothing is much larger than previously believed, suggesting that its measurement of the size of the CMBR ripples is not as accurate as was thought.
If true this could mean that the ripples are significantly smaller, which could imply that dark matter and dark energy are not present after all.
Professor Shanks said: "CMB observations are a powerful tool for cosmology and it is vital to check for systematic effects.
"If our results prove correct then it will become less likely that dark energy and exotic dark matter particles dominate the Universe. So the evidence that the Universe has a 'Dark Side' will weaken."
In addition, Durham astronomers recently collaborated in an international team whose research suggested that the structure of the CMB may not provide the robust independent check on the presence of dark energy that it was thought to.
Utane Sawangwit said: "If our result is repeated in new surveys of galaxies in the Southern Hemisphere then this could mean real problems for the existence of dark energy."
If the Universe really has no 'dark side', it will come as a relief to some theoretical physicists. Having a model dependent on as yet undetected exotic particles that make up dark matter and the completely mysterious dark energy leaves many scientists feeling uncomfortable.
It also throws up problems for the birth of stars in galaxies, with as much 'feedback' energy needed to prevent their creation as gravity provides to help them form.
Professor Shanks added: "Odds are that the standard model with its enigmatic dark energy and dark matter will survive, but more tests are needed.
"The European PLANCK satellite, currently out there collecting more CMB data will provide vital new information and help us answer these fundamental questions about the nature of the Universe we live in."