South Pole Telescope hones in on dark energy, neutrinos

April 2, 2012, University of Chicago
New data from the South Pole Telescope is bolstering Albert Einstein's cosmological constant, an idea he considered to be his greatest blunder, to explain the modern mystery of dark energy. The SPT collaboration's latest analyses have been submitted to the Astrophysical Journal and was presented April 1 at the American Physical Society meeting in Atlanta. Credit: Daniel Luong-Van

Analysis of data from the 10-meter South Pole Telescope is providing new support for the most widely accepted explanation of dark energy — the source of the mysterious force that is responsible for the accelerating expansion of the universe.

The results also are beginning to hone in on the masses of neutrinos, the most abundant particles in the universe, which until recently were thought to be without mass.

The data strongly support the leading model for , Albert Einstein's cosmological constant — a slight modification to his theory of general relativity — even though the analysis was based on only a fraction of the SPT data collected and only 100 of the more than 500 detected so far.

"With the full SPT data set, we will be able to place extremely tight constraints on dark energy and possibly determine the mass of the neutrinos," said Bradford Benson, a postdoctoral scientist at the University of Chicago's Kavli Institute for Cosmological Physics. Benson presented the SPT collaboration's latest findings on April 1 at the American Physical Society meeting in Atlanta.

A series of papers detailing the SPT findings have been submitted to the Astrophysical Journal (see ApJ, 2011, 743, 28 led by Ryan Keisler, led by Benson, and led by Christian Reichardt).

The results are based on a new method that combines measurements taken by the SPT and X-ray satellites, and extends these measurements to larger distances than previously achieved using galaxy clusters.

The most widely accepted property of dark energy is that it leads to a pervasive force acting everywhere and at all times in the universe. This force could be the manifestation of Einstein's cosmological constant, which effectively assigns energy to empty space, even when it is free of matter and radiation.

Einstein introduced the cosmological constant into his theory of general relativity to accommodate a stationary universe, the dominant idea of his day. He later considered it to be his greatest blunder after the discovery of an expanding universe.

In the late 1990s, astronomers discovered that the expansion of the universe appeared to be accelerating, according to cosmic distance measurements based on the brightness of exploding stars. Gravity should have been slowing the expansion, but instead it was speeding up.

Einstein's is one explanation of the observed acceleration of the expanding universe, now supported by countless astronomical observations. Others hypothesize that gravity could operate differently on the largest scales of the universe. In either case, the astronomical measurements are pointing to new physics that have yet to be understood.

This image displays a portion of the South Pole Telescope survey of the cosmic microwave background (CMB) - the radiant light left over from the Big Bang. Points of light mark quasars and gravitationally lensed galaxies. The variations in the image are minute fluctuations in the intensity of the CMB. The fluctuations are caused by differences in the distribution of matter in the early universe at a time only 400,000 years after the Big Bang. The image is effectively a "baby picture" of the universe. Credit: SPT Collaboration
Clues to dark energy lurking in 'shadows'

The SPT was specifically designed to tackle the dark energy mystery. The 10-meter telescope operates at millimeter wavelengths to make high-resolution images of the cosmic microwave background radiation (CMB), the light left over from the big bang. Scientists use the CMB in their search for distant, massive galaxy clusters, which can be used to pinpoint the mass of the neutrino and the properties of dark energy.

"The CMB is literally an image of the universe when it was only 400,000 years old, from a time before the first planets, stars and galaxies formed in the universe," Benson said. "The CMB has travelled across the entire observable universe, for almost 14 billion years, and during its journey is imprinted with information regarding both the content and evolution of the universe."

As the CMB passes through galaxy clusters, the clusters effectively leave "shadows" that allow astronomers to identify the most massive clusters in the universe, nearly independent of their distance.

"Clusters of galaxies are the most massive, rare objects in the universe, and therefore they can be effective probes to study physics on the largest scales of the universe," said John Carlstrom, the S. Chandrasekhar Distinguished Service Professor in Astronomy & Astrophysics, who heads the SPT collaboration.

"The unsurpassed sensitivity and resolution of the CMB maps produced with the provides the most detailed view of the young universe and allows us to find all the massive clusters in the distant universe," said Christian Reichardt, a postdoctoral researcher at the University of California, Berkeley, and lead author of the new SPT cluster catalog paper.

The number of clusters that formed over the history of the universe is sensitive to the mass of neutrinos and the influence of dark energy on the growth of cosmic structures.

"Neutrinos are amongst the most abundant particles in the universe," Benson said. "About one trillion neutrinos pass through us each second, though you would hardly notice them because they rarely interact with 'normal' matter."

The existence of neutrinos was proposed in 1930. They were first detected 25 years later, but their exact mass remains unknown. If they are too massive they would significantly affect the formation of galaxies and galaxy clusters, Benson said.

The SPT team has now placed tight limits on the neutrino masses, yielding a value that approaches predictions stemming from particle physics measurements.

"It is astounding how SPT measurements of the largest structures in the lead to new insights on the evasive neutrinos," said Lloyd Knox, professor of physics at the University of California at Davis and member of the SPT collaboration. Knox also will highlight the neutrino results in his presentation on in Cosmology at a special session of the APS on April 3.

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2.9 / 5 (7) Apr 02, 2012
Damnit all to hell, it's "homes in on," not "hones in on". Get a literate proofreader. I know, you don't think it matters, but it does -- mistakes like this undermine your credibility WAY more than a page full of typos would.

3.8 / 5 (4) Apr 02, 2012
A quick search and you will find that either is acceptable.

Try ...


5 / 5 (1) Apr 02, 2012
Take it easy on them, man! I get tired of you guys drilling the creators of this site for tiny details. This is a New PORTAL site, meaning they usually take info from other articles on other sites. Often this is the source of the errors. Anyway, stop bickering and keep reading this awesome website!

I hope they can figure out the nature of the universe, and what is up with neutrinos? Are they linked to something else, link other dimensions?
1 / 5 (4) Apr 02, 2012
I hope they can figure out the nature of the universe, and what is up with neutrinos? Are they linked to something else, link other dimensions?
In order for someone to go from one dimension of space to another one has to go through DM to get there. One will not be able to go directly from here (atoms) to get there (another dimension of space).
5 / 5 (1) Apr 02, 2012
A thought occurs to me, if neutrinos are affected by gravity, can they be slowed down and even reversed by galactic gravity? How easy is it to detect a "slow" neutrino? Can their numbers be more difficult to estimate if we cant detect a neutrino that is slow?
5 / 5 (1) Apr 03, 2012
@Sanescience - Neutrinos are so low rest mass and go so close to the speed of light that it is very hard for gravity to slow them down much.
If gravity (or anything else) steals 99% of the energy of a non-relativistic particle, its speed is reduced by 90%.
But if gravity (such as being produced close to a black hole) steals 90% of the energy of a neutrino at 99.999999% of the speed of light, it will still be going at 99.99999% of the speed of light.

We don't know how close to massless neutrinos are and thus how close to the speed of light they are going for a given energy, But we do know that they are very low mass and moving very close to the speed of light.

A long way of saying that it is hard for gravity even to steal much energy from a neutrino, and very much harder for it to steal much velocity.
not rated yet Apr 04, 2012
The image of the CMB seems to have a variety of structures, eg filaments or several filaments radiating out from a point. And there are also some straight lines, hopefully not artifacts. There is also a speckley appearance (which may be due to noise).

I would also be interested to see if the CMB is cooling over time. It should be decreasing in temperature in proportion to time elapsed, so after 14 years I would expect one part in a billion decrease.

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