Astronomers confirm Einstein’s theory of general relativity

Washington, March 26 (ANI): An international team of astronomers has confirmed Albert Einstein’s theory of general relativity and that the expansion of the universe is accelerating after looking at data from the largest-ever survey conducted by the Hubble Space Telescope.

The astronomers studied more than 446,000 galaxies to map the matter distribution and the expansion history of the universe.

This study enabled them to observe precisely how dark matter evolved in the universe and to reconstruct a three-dimensional map of the dark matter and use this to test Albert Einstein’s theory of general relativity.

“Our results confirmed that there is an unknown source of energy in the universe which is causing the cosmic expansion to speed up, stretching the dark matter further apart exactly as predicted by Einstein’s theory,” said Van Waerbeke, an associate professor in the Dept. of Physics and Astronomy.

Einstein’s theory of general relativity predicts that space and time is a soft geometrical structure of which the shape and evolution are entirely determined by the matter within it.

Scientists posit that the universe is composed of dark matter and normal matter with a third constituent called “dark energy,” which over the past two billion years has been the force behind the accelerated expansion of the universe.

“The data from our study are consistent with these predictions and show no deviation from Einstein’s theories,” said Van Waerbeke, who is also a scholar in the Cosmology and Gravity program of the Canadian Institute for Advanced Research. (ANI)

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)