Why a Pile of Odd-Shaped Particles Doesn't Collapse ✎ express

Original: "Origin of geometric cohesion in non-convex granular materials: interplay between interdigitation and rotational constraints enhancing frictional stability"
arXiv:2601.00262 · 2026-01-01 · CC BY-NC-SA 4.0 · independent analysis · 1 min
Scientists peered inside sand piles made of strangely shaped particles and figured out what holds them together.

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Pour a handful of dry sand: it will spread into a neat cone. Now grab a box of star-shaped pasta: the pile will stand almost vertical. Why? It's all about particle shape.

Physicists built cylindrical piles from particles of different geometries — from smooth spheres to 'polypods' with several arms, like a sea star. Each pile was scanned with an X-ray tomograph to see the position, orientation, and contacts of every particle. It turned out that for particles with protrusions, neighbors interlock like fingers of clasped hands, preventing each other from moving. Even without glue or friction, such a pile holds its shape.

The most stable configuration is particles with three or more arms: they form locks that don't come undone under their own weight.

The scientists derived a simple parameter: it accounts for how many contacts each particle has and how they are arranged. This parameter accurately predicted whether a pile would stand or collapse. This means you can calculate in advance which particle shape to choose so that an embankment, a pill, or a construction mix is as strong as possible.

In nature, sand wasps use a similar trick: they build nests from sand grains with sharp edges, and the nest holds together without any cement.

Scientists
William Lawrence Bragg
Concepts
quark structure probing microparticle protein structure gravitational interaction accretion disk nuclear shape gravitational instability planetary composition formation self assembly Accretion disk geometry planetary interior porous material planetesimal formation biofilm dust dynamics crystal growth intercalation materials science topological protection innermost stable circular orbit