In a special scale-invariant fracton Hamiltonian, late-time attractors reproduce the scale expansion, homogeneity, critical Newtonian dynamics, and arrow of time of a flat matter-dominated cosmology.
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Classical fractons with cosmological fixed points
In a special scale-invariant fracton Hamiltonian, late-time attractors reproduce the scale expansion, homogeneity, critical Newtonian dynamics, and arrow of time of a flat matter-dominated cosmology.