Atomistic simulations of the vertical propagation of perturbations in deep gravitationally compacted granular columns characterized by the intergrain potential V(δ)∝δⁿ, with n≥2 and δ the grain overlap, are shown to recover the results of elasticity theory for weak perturbations. For strong perturbations, the sound velocity cstrong→cweak as z→∞ with the deviations from cweak best expressed via a certain recursion relation in z. We predict that voids in real granular columns lead to c∝1-ε, when the void fraction ε is small, and show that the velocity power spectrum of a grain resembles that of a harmonic oscillator chain as z→∞.
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Sinkovits et al. (1995) studied this question.
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