What if the largest structures in the Universe aren’t just expanding — but spinning?
In this episode, host Paul Adepoju explores one of the most intriguing recent developments in cosmology: evidence that a vast cosmic filament stretching tens of millions of light-years may be rotating. The conversation builds on Paul’s feature for Physics Magazine, originally developed as the winning pitch of the Quantum Pitch Competition — launched by Physics Magazine in partnership with Physics World to mark the International Year of Quantum Science and Technology. His article described how astronomers detected large-scale galactic motion using radiation produced by tiny quantum “spin flips” in hydrogen atoms. Read it here.
Drawing on that reporting and an in-depth interview with astrophysicist Dr. Madalina Tudorache, this episode examines how galaxies align along cosmic filaments, how neutral-hydrogen observations reveal coordinated motion, and why angular momentum at these scales is reshaping questions about galaxy formation and large-scale structure.
Along the way, we connect quantum-scale measurements — the 21-centimeter hydrogen transition — to observations of the cosmic web, discuss the role of South Africa’s MeerKAT telescope in enabling the discovery, and reflect on how global collaboration and African radio-astronomy infrastructure are influencing frontier astrophysics.
This episode unpacks the discovery, the physics behind it, and the broader story of how we come to understand motion across the Universe.
