Synthetic rotation brings black hole energy theory into lab, amplifying waves

Researchers at the CUNY Graduate Center have developed a radio-frequency device that simulates the extreme rotational speeds of a black hole. This synthetic approach allows scientists to study wave amplification and energy extraction in a laboratory setting.
Why it matters
This breakthrough provides a new experimental method to test complex astrophysical theories regarding black holes that were previously impossible to observe directly.
edited by Gaby Clark , reviewed by Andrew Zinin
This article has been reviewed according to Science X's editorial process and policies . Editors have highlighted the following attributes while ensuring the content's credibility:
Add as preferred source Floquet-based rotation and rotational super-radiance. Credit: Nature (2026). DOI: 10.1038/s41586-026-10725-y More than half a century ago, Sir Roger Penrose envisioned a scenario in which energy could be extracted from a black hole spinning at extreme speeds. He proposed that a particle entering its ergosphere—a region of space dragged around by a rotating black hole—could split into two. One part could fall into the black hole while the other escaped carrying more energy than the original particle. Building on this theory, physicist Yakov Zel'dovich later predicted that a wave interacting with a sufficiently fast, rotating object could extract energy from it and become amplified.
Get smarter about the news
Sign up free for a feed built around what you actually care about, Dive Deeper research on any story, and the full text of every article.
Create free accountAlready have an account? Sign in