For those not overly enamored with the power of entropy to drive order, or how tightly you can pack your d4 die into your bag of holding, the implications of this work go deeper than you might expect.

We point out that two problems of observational cosmology, namely the facts (i) that ≳60 per cent of the baryonic content of the Universe is not observed at z∼ 0 and (ii) that the properties of small ...