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Ripples in the Cosmic Web

Ripples in the Cosmic Web

Credit: J. Onorbe /MPIA

Volume rendering of the output from a supercomputer simulation showing part of the cosmic web, 11.5 billion years ago. This and other models of the universe were generated and directly compared with quasar pair data in order to measure the small-scale ripples in the cosmic web. The cube is 24 million light years on a side.

Ripples in the Cosmic Web

Credit: Springel et al. (2005) (cosmic web)/J. Neidel, MPIA

Schematic representation of the technique used to probe the small-scale structure of the cosmic web using light from a rare quasar pair. The spectra (bottom right) contain information about the hydrogen gas the light has encountered, as well as the distance of that gas.

Ripples in the Cosmic Web

Credit: Rorai et al./MPIA

Spectra of both members of a close quasar pair used in the study. The subtle differences in the absorption features between the two sight lines allow the researchers to probe the small-scale structure of the cosmic web.

MEDIA CONTACT:

Mari-Ela Chock, Communications Officer

W. M. Keck Observatory

(808) 554-0567

mchock@keck.hawaii.edu


SCIENCE CONTACTS:

Alberto Rorai, Lead Author

University of Cambridge

+44 01223 746433

arorai@ast.cam.ac.uk

Joseph Hennawi, Co-author

University of California - Santa Barbara

(805) 893-3503

joe@physics.ucsb.edu

Maunakea, Hawaii – Astronomers for the first time have measured small ripples in the cosmic web using W. M. Keck Observatory images of rare double quasars.

The most barren regions of the universe are the far-flung corners of intergalactic space. In these vast expanses between the galaxies there is just one solitary atom per cubic meter — a diffuse haze of hydrogen gas left over from the Big Bang.

On the largest scales, this diffuse material is arranged in a vast network of filamentary structures known as the “cosmic web,” its tangled strands spanning billions of light years and accounting for the majority of atoms in the universe.

Now, a team of astronomers has made the first measurements of small-scale ripples in this primeval hydrogen gas. Although the regions of cosmic web they studied lie nearly 11 billion light years away, they were able to measure variations in its structure on scales 100,000 times smaller, comparable to the size of a single galaxy. The results appear in the journal Science.

Intergalactic gas is so tenuous that it emits no light of its own. Instead astronomers study it indirectly by observing how it selectively absorbs the light coming from faraway sources known as quasars.

Quasars constitute a brief hyperluminous phase of the galactic life-cycle powered by the infall of matter onto a galaxy’s central supermassive black hole. Quasars act like cosmic lighthouses — bright, distant beacons that allow astronomers to study intergalactic atoms residing between the location of the quasar and the Earth.

But because these hyperluminous episodes last only a tiny fraction of a galaxy’s lifetime, quasars are correspondingly rare on the sky and are typically separated by hundreds of millions of light years from each other.

In order to probe the cosmic web on much smaller length scales, the astronomers exploited a fortuitous cosmic coincidence: They identified exceedingly rare pairs of quasars right next to each other on the sky and measured subtle differences in the absorption of intergalactic atoms measured along the two sightlines.

“Pairs of quasars are like needles in a haystack. In order to find them we combed through images of billions of celestial objects, millions of times fainter than what the naked eye can see,” explains Joseph Hennawi, an associate professor at University of California Santa Barbara’s Department of Physics.

Hennawi pioneered the application of algorithms from ‘machine learning’, a branch of artificial intelligence, to efficiently locate quasar pairs in the massive amounts of data produced by digital imaging surveys of the night sky.

Once identified, the quasar pairs were observed with the largest telescopes in the world, including the 10-meter telescopes at the W. M. Keck Observatory on Maunakea, Hawaii. The University of California (UC) is a founding partner of Keck Observatory, and UC astronomers have access to its telescopes.

The discovery team gathered a majority of the data using the Low Resolution Imaging Spectrometer (LRIS), a faint-light instrument on the Keck I telescope capable of taking spectra and images of the most distant known objects in the universe, along with the Echellette Spectrograph and Imager (ESI) on Keck II to capture high-resolution spectra of the rare double quasars.

“One of the biggest challenges was developing the mathematical and statistical tools to quantify the tiny differences we measured in this new kind of data,” said lead author Alberto Rorai, Hennawi’s former PhD student, who is now a postdoctoral researcher at Cambridge University. Rorai developed these tools as part of the research for his doctoral degree, and applied them to spectra of quasars obtained with Hennawi and other colleagues.

The astronomers compared their measurements to supercomputer models that simulate the formation of cosmic structures from the Big Bang to the present.

“The input to our simulations are the laws of physics and the output is an artificial universe, which can be directly compared to astronomical data,” said co-author Jose Oñorbe, a postdoctoral researcher at the Max Planck Institute for Astronomy who led the supercomputer simulation effort. “I was delighted to see that these new measurements agree with the well-established paradigm for how cosmic structures form.”

On a single laptop, these complex calculations would have required almost 1,000 years to complete, but modern supercomputers enabled the researchers to carry them out in just a few weeks.

“One reason these small-scale fluctuations are so interesting is that they encode information about the temperature of gas in the cosmic web just a few billion years after the Big Bang,” explained Hennawi.

Astronomers believe that the matter in the universe went through phase transitions billions of years ago, which dramatically changed its temperature. These phase transitions, known as cosmic re-ionization, occurred when the collective ultraviolet glow of all stars and quasars in the universe became intense enough to strip electrons off atoms in intergalactic space.

How and when re-ionization occurred is one of the biggest open questions in the field of cosmology, and these new measurements provide important clues that will help narrate this chapter of the history of the universe.

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About W. M. Keck Observatory

The W. M. Keck Observatory operates the largest, most scientifically productive telescopes on Earth. The two, 10-meter optical/infrared telescopes on the summit of Maunakea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrometers, and world-leading laser guide star adaptive optics systems. The Observatory is a private 501(c) 3 non-profit organization and a scientific partnership of the California Institute of Technology, the University of California, and NASA.