How to handle the inelastic collapse of a dissipative hard-sphere gas with the TC model

Stefan Luding*, Sean McNamara

*Corresponding author for this work

    Research output: Contribution to journalArticleAcademicpeer-review

    123 Citations (Scopus)

    Abstract

    The inelastic hard sphere model of granular material is simple, easily accessible to theory and simulation, and captures much of the physics of granular media. It has three drawbacks, all related to the approximation that collisions are instantaneous: 1) The number of collisions per unit time can diverge, i.e. the "inelastic collapse" can occur. 2) All interactions are binary; multiparticle contacts cannot occur and 3) no static limit exists. We extend the inelastic hard sphere model by defining a duration of contact tc such that dissipation is allowed only if the time between contacts is larger than tc. We name this generalized model the TC model and discuss it using examples of dynamic and static systems. The contact duration used here does not change the instantaneous nature of the hard sphere contacts, but accounts for a reduced dissipation during "multiparticle contacts". Kinetic and elastic energies are denned as well as forces and stresses in the system. Finally, we present event-driven numerical simulations of situations far beyond the inelastic collapse, possible only with the TC model.

    Original languageEnglish
    Pages (from-to)113-128
    Number of pages16
    JournalGranular matter
    Volume1
    Issue number3
    DOIs
    Publication statusPublished - 1 Jan 1998

    Keywords

    • Event driven simulations; kinetic theory
    • Inelastic collapse
    • Inelastic hard sphere model

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