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News — Gravity has shaped our cosmos. Its attractive influence turned tiny variations in the amount of matter present in the early Universe into the sprawling strands of galaxies we see today. A new study using the first year of data from the Dark Energy Spectroscopic Instrument () has traced how this cosmic structure grew over the past 11 billion years, providing the most precise test to date of how gravity behaves at very large scales.

DESI is a state-of-the-art instrument that can capture light from 5000 galaxies simultaneously. It was constructed, and is operated, with funding from the DOE Office of Science. DESI is mounted on the U.S. National Science Foundation at , a Program of NSF NOIRLab. The program is now in its fourth of five years surveying the sky and is set to observe roughly 40 million galaxies and quasars by the time the project ends.

The DESI project is an international collaboration of more than 900 researchers from over 70 institutions around the world and is managed by the Department of Energy’s Lawrence Berkeley National Laboratory ().

In their new study, DESI researchers found that gravity behaves as predicted by . The result validates our leading model of the Universe and limits possible theories of , which have been proposed as alternative ways to explain unexpected observations, such as the accelerating expansion of our Universe that is typically attributed to [1].

The DESI collaboration shared their results in posted to the online repository arXiv today. The complex analysis used nearly six million galaxies and and lets researchers see up to 11 billion years into the past. With just one year of data, DESI has made the most precise overall measurement of the growth of cosmic structure, surpassing previous efforts that took decades to complete.

Today’s results provide an extended analysis of DESI’s first year of data, which made the largest 3D map of our Universe to date and revealed hints that dark energy might be evolving over time. The April results looked at a particular feature of how galaxies cluster known as baryon acoustic oscillations (). The new analysis broadens the scope by measuring how galaxies and matter are distributed on different scales throughout space. The study also provided improved constraints on the mass of [2], the only fundamental particles whose masses have not yet been precisely measured. Neutrinos influence the clustering pattern of galaxies very slightly but this can be measured with the quality of the DESI data. The DESI constraints are the most stringent to date, complementing constraints from laboratory measurements.

The study required months of additional work and cross-checks. Like the previous study, it used a technique to hide the result from the scientists until the end, mitigating any unconscious bias. 

“This research is part of one of the key projects of the DESI experiment — to learn about the fundamental aspects of our Universe at large scales, such as matter distribution and the behavior of dark energy, as well as fundamental aspects of particles,” says Stephanie Juneau, NSF NOIRLab astronomer and a member of the DESI collaboration. “By comparing the evolution of the matter distribution in the Universe with existing predictions, including Einstein’s theory of general relativity and competing theories, we're really tightening the possibilities on our models of gravity.”

The collaboration is currently analyzing the first three years of collected data and expects to present updated measurements of dark energy and the expansion history of our Universe in the coming year. DESI’s expanded results released today are consistent with the experiment’s earlier preference for an evolving dark energy, adding to the anticipation of the upcoming analysis.

“Dark matter makes up about a quarter of the Universe, and dark energy makes up another 70 percent, and we don’t really know what either one is,” said Mark Maus, a PhD student at Berkeley Lab and UC Berkeley who worked on theory and validation modeling pipelines for the new analysis. “The idea that we can take pictures of the Universe and tackle these big, fundamental questions is mind-blowing.”

While the DESI year-one data are not yet publicly available, researchers can access the early data release. It is available as and as searchable databases of catalogs and spectra via the and at the Community Science and Data Center, a Program of NSF NOIRLab.

Notes

[1] The accelerating expansion of the Universe and discovery of dark energy was a revolutionary advancement in cosmology. The NOIRLab facilities supporting both with instrumentation and telescopes to do the detailed measurements of supernovae that led to this discovery.

[2] Previous neutrino experiments found that the sum of the masses of the three types of neutrinos should be at least 0.059 eV/c2. (For comparison, an electron has a mass of about 511,000 eV/c2.) DESI’s results indicate that the sum should be less than 0.071 eV/c2, leaving a narrow window for neutrino masses.

More information

DESI is supported by the DOE Office of Science and by the National Energy Research Scientific Computing Center, a DOE Office of Science user facility. Additional support for DESI is provided by the U.S. National Science Foundation; the Science and Technology Facilities Council of the United Kingdom; the Gordon and Betty Moore Foundation; the Heising-Simons Foundation; the French Alternative Energies and Atomic Energy Commission (CEA); the National Council of Humanities, Sciences, and Technologies of Mexico; the Ministry of Science and Innovation of Spain; and by the DESI member institutions.

The DESI collaboration is honored to be permitted to conduct scientific research on I’oligam Du’ag (Kitt Peak), a mountain with particular significance to the Tohono O’odham Nation.

(U.S. National Science Foundation National Optical-Infrared Astronomy Research Laboratory), the U.S. center for ground-based optical-infrared astronomy, operates the (a facility of , , , , , and ), NSF Kitt Peak National Observatory (), NSF Cerro Tololo Inter-American Observatory (), the Community Science and Data Center (), and (operated in cooperation with the ’s National Accelerator Laboratory). It is managed by the Association of Universities for Research in Astronomy () under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on I’oligam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawai‘i, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O’odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.

(Berkeley Lab) is committed to delivering solutions for humankind through research in clean energy, a healthy planet, and discovery science. Founded in 1931 on the belief that the biggest problems are best addressed by teams, Berkeley Lab and its scientists have been recognized with 16 Nobel Prizes. Researchers from around the world rely on the lab’s world-class scientific facilities for their own pioneering research. Berkeley Lab is a multiprogram national laboratory managed by the University of California for the U.S. Department of Energy’s Office of Science.

DOE’s Office of Science is the single largest supporter of basic research in the physical sciences in the United States, and is working to address some of the most pressing challenges of our time. For more information, please visit .

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