New Study Reveals How Spacetime Crystals Can Lead to Black Hole Formation
When Spacetime Crystallises, a Black Hole is Born

Image: Universe Today
Researchers from TU Wien and Goethe University Frankfurt have derived a mathematical formula showing that spacetime can crystallize, leading to the formation of black holes. This process, termed critical collapse, occurs at a delicate balance point of spacetime, where a slight energy addition can trigger the collapse into a black hole.
- 01The study published in *Physical Review Letters* presents a mathematical formula for spacetime crystals, which can lead to black holes.
- 02Black holes traditionally form from the collapse of massive stars, but microscopic black holes can emerge from a critical state of spacetime.
- 03The process of critical collapse occurs when spacetime organizes into a repeating pattern, tipping into a black hole with a small energy input.
- 04The research team utilized a novel approach by solving equations in infinitely many dimensions, simplifying the complex problem.
- 05This breakthrough offers a new analytical method for studying black hole phenomena that were previously difficult to analyze.
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A recent study from researchers at TU Wien in Vienna and Goethe University Frankfurt has uncovered a fascinating phenomenon where spacetime can crystallize, potentially leading to the formation of black holes. Published in *Physical Review Letters*, the study introduces a mathematical formula that describes these theoretical spacetime crystals. Unlike traditional black holes, which form from the collapse of massive stars, microscopic black holes can arise from a delicate balance in spacetime, termed critical collapse. This occurs when spacetime organizes into a structured pattern and, with the slightest addition of energy, collapses into a black hole. The researchers employed a novel approach by solving the problem in infinitely many dimensions, which simplified the mathematical complexities involved. Florian Ecker from TU Wien noted that this technique provides a stable method for studying black hole-related phenomena that were previously analytically intractable. This groundbreaking work not only advances theoretical physics but also opens new avenues for understanding the nature of black holes.
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