New Scientist - 11 June 2010
It's supposed to be the "gold standard" of evidence supporting the standard model of cosmology – including dark matter, dark energy and the exponential expansion after the big bang known as inflation.
But could it be wrong? Might misleading measurements by NASA's Wilkinson Microwave Anisotropy Probe (WMAP) have been leading us towards the wrong theory of cosmology? One astrophysicist thinks so, and he says the planet Jupiter is to blame – though others insist that there is nothing amiss.
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To calibrate the microwave data, WMAP scientists use the planet Jupiter, which they assume to be a steady source of microwaves. Observations of Jupiter show how much the cosmic ripples are being blurred by the instrument's optics, allowing the WMAP team to correct for this.
Now Shanks and his PhD student Utane Sawangwit have recalibrated the data using objects such as radio galaxies observed by WMAP that also emit microwaves. The result is a spectrum that is compatible with a host of theories that the WMAP team claims to have ruled out. For example, one-dimensional cosmic strings – defects in the fabric of space-time – or modified laws of gravity might explain the clumping of matter that is currently attributed to the dark matter and dark energy of the standard model.
Durham astronomers' doubts about the 'dark side'
Royal Astronomical Society - RAS PN 10/44 - 14 June 2010
New research by astronomers in the Physics Department at Durham University suggests that the conventional wisdom about the content of the Universe may be wrong. Graduate student Utane Sawangwit and Professor Tom Shanks looked at observations from the Wilkinson Microwave Anisotropy Probe (WMAP) satellite to study the remnant heat from the Big Bang. The two scientists find 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. The team publish their results in a letter to the journal Monthly Notices of the Royal Astronomical Society.
Launched in 2001, WMAP measures differences in the 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 is made up of 4% ‘normal’ matter, 22% ‘dark’ or invisible matter and 74% ‘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 find 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.
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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.
If dark energy does exist, then it ultimately causes the expansion of the Universe to accelerate. On their journey from the CMB to the telescopes like WMAP, photons (the basic particles of electromagnetic radiation including light and radio waves) travel through giant superclusters of galaxies. Normally a CMB photon is first blueshifted (its peak shifts towards the blue end of the spectrum) when it enters the supercluster and then redshifted as it leaves, so that the two effects cancel. However, if the supercluster galaxies are accelerating away from each other because of dark energy, the cancellation is not exact, so photons stay slightly blueshifted after their passage. Slightly higher temperatures should appear in the CMB where the photons have passed through superclusters.
However, the new results, based on the Sloan Digital Sky Survey which surveyed 1 million luminous red galaxies, suggest that no such effect is seen, again threatening the standard model of the Universe.
Beam profile sensitivity of the WMAP CMB power spectrum
- arXiv.org > astro-ph > arXiv:0912.0524 > 02 Dec 2009 (v1), 08 Jun 2010 (v2)
to be published in Monthly Notices of the Royal Astronomical Society: Letters