Low-speed impact craters in loose granular media

dc.creatorUehara, J. S.
dc.creatorAmbroso, M. A.
dc.creatorOjha, R. P.
dc.creatorDurian, D. J.
dc.date2003-01-28
dc.date2003-03-25
dc.date.accessioned2026-07-07T02:49:24Z
dc.date.available2026-07-07T02:49:24Z
dc.descriptionWe report on craters formed by balls dropped into dry, non-cohesive, granular media. By explicit variation of ball density $ρ_{b}$, diameter $D_{b}$, and drop height $H$, the crater diameter is confirmed to scale as the 1/4 power of the energy of the ball at impact: $D_{c}\sim(ρ_{b}{D_{b}}^{3}H)^{1/4}$. Against expectation, a different scaling law is discovered for the crater depth: $d\sim({ρ_{b}}^{3/2}{D_{b}}^{2}H)^{1/3}$. The scaling with properties of the medium is also established. The crater depth has significance for granular mechanics in that it relates to the stopping force on the ball.
dc.descriptionexperiment; 4 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/cond-mat/0301549
dc.identifierhttp://arxiv.org/abs/cond-mat/0301549
dc.identifierPhys. Rev. Lett. 90, 194301 (2003)
dc.identifierdoi:10.1103/PhysRevLett.90.194301
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/20780
dc.subjectSoft Condensed Matter
dc.titleLow-speed impact craters in loose granular media
dc.typetext

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