'Crystals' of space-time could be the origins of certain rare black holes, theoretical study hints

By taking general relativity into higher dimensions, a trio of physicists has proven that a mathematical pattern of ripples in space-time geometry could give rise to naked singularities and microscopic black holes.

An illustration of a black hole surrounded by swirling pink and blue gas in the darkness of space.
An illustration of space-time curving around a black hole. New theoretical research picks up a problem contemplated by Stephen Hawking and Kip Thorne about whether ‘naked’ singularities can emerge from rare patterns in space-time geometry.
(Image credit: MARK GARLICK/SCIENCE PHOTO LIBRARY via Getty Images)

A new theoretical study adds fresh support to the idea that a mathematical pattern of ripples in space-time geometry could give rise to naked singularities and microscopic black holes. The new finding advances research into a subject that has vexed physicists for decades.

In 1997, Stephen Hawking famously conceded defeat on a 1991 bet with fellow theoretical physicists Kip Thorne and John Preskill about the possible existence of naked singularities: objects like black holes but without an event horizon (a point beyond which light, and all other matter, cannot escape), making them observable. Hawking eventually admitted that such objects could exist. Thorne and Preskill’s prize? T-shirts to cover their "nakedness."

Benjamin Skuse
Live Science contributor

Benjamin Skuse is a professional freelance writer of all things science and technology. Previously, he earned a PhD in applied mathematics from the University of Edinburgh and an MSc in science communication from the University of the West of England. His work has appeared in New Scientist, WIRED, IEEE Spectrum, Physics World, Sky & Telescope, Photonics Focus, and many more outlets.

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