Waterloo scientists have developed a new way to understand how the universe began, and it could change what we know about the Big Bang and the earliest moments of cosmic history. Their work suggests that the universe’s rapid early expansion could have arisen naturally from a deeper, more complete theory of quantum gravity.
Dr. Niayesh Afshordi, professor of physics and astronomy at the University of Waterloo and Perimeter Institute (PI), led the research team that explored a novel method of combining gravity with quantum physics, the rules that govern how the smallest particles in the universe behave. While general relativity has been successful for more than a century, it breaks down at the extreme conditions that existed at the birth of the universe. To address this problem, the team used Quadratic Quantum Gravity, which remains mathematically consistent even at extremely high energies - similar to the kind present during the Big Bang.
Most existing explanations for the Big Bang rely on Einstein’s theory of gravity, plus additional components added by hand. This new approach offers a more unified picture that connects the earliest moments of the universe to the well-tested cosmology scientists observe today.
The research team found that the Big Bang’s rapid early expansion can emerge naturally from this simple, consistent theory of quantum gravity, without adding any extra ingredients. This early burst of expansion, often called inflation, is a central idea in modern cosmology because it explains why the universe looks the way it does today.
Their model also predicts a minimum amount of primordial gravitational waves, which are tiny ripples in spacetime geometry created in the first moments after the Big Bang. These signals may be detectable in upcoming experiments, offering a rare chance to test ideas about the universe’s quantum origins.
"This work shows that the universe’s explosive early growth can come directly from a deeper theory of gravity itself," Afshordi said. "Instead of adding new pieces to Einstein’s theory, we found that the rapid expansion emerges naturally once gravity is treated in a way that remains consistent at extremely high energies."
The researchers were surprised by how testable their theory turned out to be.
"Even though this model deals with incredibly high energies, it leads to clear predictions that today’s experiments can actually look for," Afshordi said. "That direct link between quantum gravity and real data is rare and exciting."
The timing of this work is significant. Cosmology is entering a new era of precision, where new instruments can measure the universe with unprecedented accuracy. Upcoming galaxy surveys, cosmic microwave background experiments, and gravitational wave detectors are becoming sensitive enough to test ideas that were once purely theoretical. At the same time, scientists are finding limitations in the simplest models of early universe expansion, increasing the need for new approaches grounded in fundamental physics.
Ruolin Liu, a PhD candidate at Waterloo and PI, and Dr. Jerome Quintin, a lecturer at l’École de technologie supérieure and former postdoctoral scholar at Waterloo and PI, also contributed to this research. The team plans to refine their predictions for upcoming experiments to explore how their framework connects to particle physics and other puzzles about the early universe. Their long-term goal is to strengthen the bridge between quantum gravity and observational cosmology.
The paper, Ultraviolet completion of the Big Bang in quadratic gravity , appears in Physical Review Letters.
