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Cosmic Voids May Contain the Universe’s Best Secrets

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Why This Matters

Cosmic voids, vast regions with minimal matter, are emerging as crucial tools for understanding fundamental cosmic mysteries such as gravity, dark energy, and the universe's expansion rate. Advances in telescopes and simulations are enabling scientists to study these voids with unprecedented clarity, potentially unlocking answers to longstanding questions about the universe's nature and our place within it.

Key Takeaways

Nature abhors a vacuum, so the saying goes, but nobody told the universe. Space is filled with cosmic voids—vast regions mostly free of matter that have opened between dense threads of material that make up a cosmic web.

Far from being vacant backwaters with little to study, these voids may hold solutions to some of the most persistent cosmic mysteries, such as the behavior of gravity, the nature of dark energy, and the so-called Hubble tension, an observational mismatch in the expansion rate of the universe that has caused astronomers’ headaches for years.

“With voids, we have the power to tackle most of the interesting cosmological riddles,” says Alice Pisani, a research professor in cosmology working at the Centre for Particle Physics in Marseille (CPPM) of the French National Centre for Scientific Research. She adds that because there’s less interference from matter, there’s a “high signal-to-noise” ratio in terms of what researchers can observe.

The advent of new telescopes and advanced simulations has supercharged this field, inspiring a growing community of scientists worldwide to specialize in voids as unique cosmological laboratories. Some experts argue we may even live inside a colossal void, a position that may alter our view of the universe in consequential ways.

For places defined by sparseness, voids are becoming cosmological heavyweights, where the laws of physics can be observed with unusual clarity.

“From a cosmology perspective, it is a very exciting time,” Pisani says.

What Are Cosmic Voids?

Following the Big Bang, the universe was a uniform soup of subatomic particles. But over millions of years, as matter cooled and stabilized into atoms, the faint outlines of the cosmic web began to emerge.

Over billions of years, the web gravitationally pulled gas clouds, galaxy clusters, and other cosmic objects toward its scaffolding. As more matter is drawn into the web, gaps have widened between its filaments, forming voids.

Small “subvoids” can open between galaxy clusters, where they might be only 10 or 20 million light years across. But voids can get bigger. Much bigger. The Boötes Void, also known as the "Great Nothing," stretches across more than 300 million light years.

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