Planck spacecraft obtains first peek of big bang’s ‘afterglow’

London, September 18 (ANI): European Space Agency’s (ESA’s) Planck spacecraft has obtained its first peek at the afterglow of the big bang, revealing it in unprecedented detail.

The ESA spacecraft was launched into space on May 14 this year. It is observing the glow of hot gas from just 380,000 years after the big bang, called the cosmic microwave background (CMB).

According to a report in New Scientist, the detailed properties of this background may contain hints of hidden extra dimensions or multiple universes, as well as providing clues to what caused a brief, early period of incredibly rapid cosmic expansion.

Planck began surveying the microwave background on August 13, a few weeks after reaching its planned perch 1.5 million kilometres from Earth at a point called L2 and cooling its detectors to within 0.1 degrees Celsius above absolute zero.

Now, the Planck team has released the probe’s first image, an observational strip covering about 5 per cent of the sky.

Slight variations in temperature from place to place in the early universe give the image its mottled appearance.

“With a few per cent of the data in, you can see it’s working well and delivering good stuff,” said team member George Efstathiou of the University of Cambridge.

Planck is expected to provide the most detailed all-sky map of the cosmic microwave background yet, improving on the best current map, obtained by NASA’s Wilkinson Microwave Anisotropy Probe (WMAP), which launched in 2001.

Planck’s detectors have more than 10 times the sensitivity of WMAP’s, and about 2.5 times the angular resolution.

“Every strip that Planck scans, we’re getting data that is many, many times more sensitive than WMAP,” Efstathiou told New Scientist.

Although Planck was only designed to observe the sky for 15 months, the team believes it could last for more than 30 months, based on new estimates of how long its coolant will last.

The extra time will allow Planck to measure the radiation with even greater precision, since it will scan the entire sky four times – two more than originally planned. (ANI)

The Universe is flat, but not entirely

London, May 19 (ANI): In a move that is reminiscent of scientists rejecting the view held by many people in the medieval times that the Earth is flat, a team of researchers has dismissed the notion that the Universe is completely flat.

According to a report in New Scientist, when it comes to the universe, “flatness” refers to the fate of light beams traveling large distances parallel to each other.

If the universe is “flat”, the beams will always remain parallel. Matter, energy and dark energy all produce curvature in space-time, however.

If the universe’s space-time is positively curved, like the surface of a sphere, parallel beams would come together. In a negatively curved, saddle-shaped universe, parallel beams would diverge.

Thanks in part to the Wilkinson Microwave Anisotropy Probe (WMAP) satellite, which revealed the density of matter and dark energy in the early universe, most astronomers are confident that the universe is flat.

But, that view is now being questioned by Joseph Silk at the University of Oxford and colleagues, who say it’s possible that the WMAP observations have been misinterpreted.

In a research paper accepted for publication in Monthly Notices of the Royal Astronomical Society, they took data from WMAP and other cosmology experiments and analyzed it using Bayes’s theorem, which can be used to show how the certainty attached to a particular conclusion is affected by different starting assumptions.

Using modern astronomers’ assumptions, which presuppose a flat universe, they calculated the probability that the universe was in one of three states: flat, positively curved or negatively curved.

This produced a 98 per cent probability that the universe is indeed flat.

When they reran the calculation starting from a more open-minded position, however, the probability changed to 67 per cent, making a flat universe far less of a certainty than astronomers generally conclude.

“It’s a reasonable assumption that the universe isn’t entirely flat,” Silk said, adding that the calculation reveals how strongly astronomers’ prejudices can affect their conclusions.

“They’ve developed a statistically rigorous way of examining the question,” said David Spergel of Princeton University, the spokesman for WMAP.

According to Silk, astronomers need to achieve a 99.9999 per cent level of confidence on the flat universe, high enough that the case starts to look compelling no matter what the starting assumptions are.

It’s possible, however, that no measurements will ever be able to get to that level of accuracy. (ANI)

Iron-arsenic superconductors exhibit unique mechanism of superconductivity

Washington, April 30 (ANI): Physicists at the U.S. Department of Energy’s Ames Laboratory have experimentally demonstrated that the superconductivity mechanism in the recently discovered iron-arsenide superconductors is unique compared to all other known classes of superconductors.

These findings, combined with iron-arsenide’s potential good ability to carry current due to their low anisotropy, may open a door to exciting possible applications in zero-resistance power transmission.

The research, led by Ames Laboratory physicist Ruslan Prozorov, has shown that electron pairing in iron-arsenides is likely to be very different when compared to other types of known superconductors.

In superconducting materials, electrons form pairs, called Cooper pairs, below a critical temperature and these electron pairs behave identically.

The collective flow of Cooper pairs results in the most famous feature of a superconductor and the feature that draws the most interest in terms of energy efficiency: the flow of electrical current without any measurable loss of energy, or true zero resistance.

However, superconductors also have another inherent characteristic that distinguishes them from a perfect metal.

Unlike perfect metals, superconductors expel a weak magnetic field from their interiors no matter whether they are cooled in a magnetic field or whether the magnetic field is applied after cooling.

In either case, a weak magnetic field penetrates only a narrow region at a superconductor’s surface. The depth of this region is known as the London penetration depth.

“The change of the London penetration depth with temperature is directly related to the structure of the so-called superconducting gap, which in turn depends on the microscopic mechanism of how electron pairs are formed,” said Prozorov.

“London penetration depth is one of the primary experimentally measurable quantities in superconductor studies,” he added.

The variation of the London penetration depth with temperature depends on the superconducting gap structure and is already generally agreed upon in most other known classes of superconductors.

In conventional superconductors – the class made up of periodic table elements, including lead and niobium – this dependence is exponential at low temperatures.

In the high-temperature cuprate superconductors, the relationship is linear, and in magnesium-diboride superconductors, the dependence is exponential, but requires two distinct superconducting gaps to explain the data in a full temperature range.

In contrast, the Ames Laboratory research group, which includes physicists Ruslan Prozorov and Makariy Tanatar, postdoctoral researcher Catalin Martin, and graduate students, Ryan Gordon, Matt Vannette and Hyunsoo Kim, found that iron-arsenide superconductors exhibit a power-law – almost quadratic – temperature variation of penetration depth.

The Ames Lab group’s findings suggest that the iron-arsenides exhibit electron pairing different from any other known superconductor. (ANI)