Physicists Derive Exact Formula for How a 'Spacetime Crystal' Becomes a Black Hole
Researchers at Goethe University Frankfurt and TU Wien have derived, for the first time, an exact formula describing how spacetime can organize into a crystal-like pattern and then collapse into a microscopic black hole.
Step by step
- 1
Matter curves spacetime into a critical state
- 2
Curvature organizes into a repeating crystal pattern
- 3
A tiny added energy tips the balance
- 4
The spacetime crystal collapses into a black hole
Physicists at Goethe University Frankfurt and TU Wien in Vienna have derived, for the first time, an exact mathematical formula describing how spacetime can organize itself into a repeating, crystal-like pattern and then suddenly collapse into a microscopic black hole.
The researchers compared the process, called critical collapse, to water freezing into ice. "Sometimes a tiny, seemingly insignificant cause is enough to trigger a huge and dramatic change," said Prof. Daniel Grumiller of TU Wien. Just as a small drop in temperature makes water molecules snap into a regular ice crystal, matter can curve spacetime under the right conditions into a finely balanced, repeating pattern the researchers call a "."
This state is unstable: it can either dissolve back into ordinary spacetime, or, if a tiny amount of energy is added, collapse into a black hole. Conditions like these may have existed shortly after the Big Bang, when matter and energy were packed into an intensely chaotic environment, potentially producing what physicists call primordial black holes.
Computer simulations first suggested in 1993 that black holes could form this way, but physicists could not derive the underlying equations analytically for decades. The Frankfurt and Vienna team solved the problem by working the calculations in a hypothetical space with far more dimensions than our universe's four, where the mathematics becomes simpler, and then translating the solution back down to four dimensions.
Florian Ecker of TU Wien said the method is "remarkably stable" and can be refined further with additional approximation techniques. The approach gives physicists a new way to study black hole formation and other extreme behaviour of spacetime without relying entirely on computer simulations.
Terms explained
The story so far
- Astronomers Spot Three Active Black Holes in a Single Galaxy From the Early Universe
- Physicists Recreate Early-Universe Matter Using Smaller Atomic Nuclei Than Ever Before
- Chinese Team Develops Tabletop X-Ray Method to Film Fast-Moving Objects
- Austrian Team Couples Electron Microscope to Quantum Computer to Sharpen Images
- Tokyo Team Recreates the Double-Slit Experiment at Atomic Scale to Read Atom Vibrations
- Ancient 'Dark Stars' May Explain a Mysterious Hum in Spacetime
- Physicists Derive Exact Formula for How a 'Spacetime Crystal' Becomes a Black Hole
