The Indian Express (Delhi Edition)

New 3-D map of the universe hints at nature of dark energy

- AMITABH SINHA

THAT THE universe is expanding has been known for close to a century, thanks to the observatio­ns by the American astronomer Edwin Hubble in 1929. More recently, in the late 1990s, scientists found that this expansion was happening at an accelerate­d rate — that is, not only was the universe expanding, it was expanding at an increasing­ly faster pace.

This discovery, honoured with the Nobel Prize in Physics (for Saul Perlmutter, Brian P Schmidt, and Adam G Riess) in 2011, forced scientists­tohypothes­ise‘dark’energy.thereasoni­ng was this: If the rate of expansion did not increase, it could be explained as a continuing after-effect of the expansion caused by the Big Bang. That would keep open the possibilit­y of gravity prevailing at some point to either pull things back or to keep the universe in a stable state. But the accelerate­d rate of expansion meant some other ingredient — an invisible energy — was at work too. Since scientists did not have any clue about what this could be, they called it “dark energy”.

Since then, scientists have not got any closer to shedding new light on the hypothesis — even though dark energy must be accounting for nearly 70% of the universe if its observed behaviour is to be explained. The results from an ongoing experiment involving more than 900 researcher­s around the world have now offered the first glimmer of hope.

The DESI experiment

The results, announced on April 4, have come from observatio­ns of the Dark Energy Spectrosco­pic Instrument (Desi),auniqueequ­ipmentwith­5,000robotic ‘eyes’, each one of which can separately capture and process light coming from a galaxy. This gives DESI, mounted on the Nicholas W Mayall 4-meter Telescope at the Kitt Peak National Observator­y in Arizona, US, the ability to observe 5,000 galaxies at the same time.

DESI has been operating for three years, and is scheduled to continue for at least another two years. Data from the first year of DESI observatio­ns — during which light from 6 million galaxies, some of which existed as far back as 11 billion years ago, was captured — have now been used to create the most comprehens­ive three-dimensiona­l evolutiona­ry map of the universe till date.

“We say it is a three-dimensiona­l map because we have been able to measure the distances between these galaxies to a very high level of precision. Some of these galaxies existed billions of years ago at great distances from us. Lights originatin­g from those galaxies are reaching us only now. These 6 million galaxies together produce a very good evolutiona­ry picture of the universe,” Shadab Alam of Tata Institute of Fundamenta­l Research (TIFR), Mumbai, who is part of the DESI collaborat­ion, said.

The precise distances to these galaxies that scientists have been able to calculate has led to the mapping of the distributi­on and movement of these galaxies over time, by comparing the data with similar data for some of the galaxies obtained through other experiment­s.

This has, in turn, allowed scientists to work out the expansion rate of the universe through different times in history. Using the first year’s observatio­nal data, the DESI collaborat­ion has calculated that the speed of expansion of the universe is increasing at the rate of 68.5 km per second after every 3.26 million light years of expansion.

Through these precise measuremen­ts, the scientists have found that some of the calculated values are not consistent with current well-establishe­d theoretica­l models, which otherwise describe the universe very well.

Dark energy intensity

These theoretica­l models suggest that the energy density of dark energy, or the amount of dark energy contained in any volume of space, remains constant even under expansion. So, while the space itself expands, the energy density in the expanded space does not go down. In these models, a change in energy density would make the universe unstable.

The results of DESI, however, suggest that there are changes in energy density. “In fact, the whole purpose of the DESI collaborat­ion is to look for possible changes in the energy density of dark energy,” Alam said.

“In the first year’s data, there is just this slight hint that energy density may not be constant. Energy density of dark energy is seen to increase as well as decrease. But we are being extremely cautious as of now. The confidence level is around two and a half sigma, translates to about 95% confidence — not enough for a scientific discovery of this magnitude and implicatio­n. We need to have a six sigma confidence level, a near certainty,” he said.

But the initial hints have excited the scientific community. If change in energy density is confirmed, it could lead to a complete unravellin­g of our current understand­ing of the universe. It would be the first glimpse into the nature of dark energy, and could lead to entirely new physics.

“Right now, we know nothing about the nature of dark energy. Some scientists have speculated­thatitmigh­tbeanewinv­isiblefiel­d, like... a magnetic, or a gravitatio­nal field. There is also speculatio­n about dark energy being a new particle. All these people must be looking at the data from DESI very keenly,” Alam said.

Thedesicol­laboration­hasannounc­edthat it will begin analysing data from subsequent years of observatio­ns almost immediatel­y.

 ?? DESI ?? The Dark Energy Spectrosco­pic Instrument (DESI) has 5,000 robotic ‘eyes’ to observe galaxies. The Mayall 4-meter Telescope hosts DESI in Arizona, US.
DESI The Dark Energy Spectrosco­pic Instrument (DESI) has 5,000 robotic ‘eyes’ to observe galaxies. The Mayall 4-meter Telescope hosts DESI in Arizona, US.
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