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    Validating N-body code chrono for granular DEM simulations in reduced-gravity environments

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    Author
    Sunday, Cecily
    Murdoch, Naomi
    Tardivel, Simon
    Schwartz, Stephen R
    Michel, Patrick
    Affiliation
    Univ Arizona, Lunar & Planetary Lab
    Issue Date
    2020-08-18
    Keywords
    methods: numerical
    planets and satellites: general
    planets and satellites: surfaces
    software: simulations
    software: development
    
    Metadata
    Show full item record
    Publisher
    OXFORD UNIV PRESS
    Citation
    Sunday, C., Murdoch, N., Tardivel, S., Schwartz, S. R., & Michel, P. (2020). Validating N-body code CHRONO for granular DEM simulations in reduced-gravity environments. Monthly Notices of the Royal Astronomical Society, 498(1), 1062-1079.
    Journal
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
    Rights
    © 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    The Discrete Element Method (DEM) is frequently used to model complex granular systems and to augment the knowledge that we obtain through theory, experimentation, and real-world observations. Numerical simulations are a particularly powerful tool for studying the regolith-covered surfaces of asteroids, comets, and small moons, where reduced-gravity environments produce ill-defined flow behaviours. In this work, we present a method for validating soft-sphere DEM codes for both terrestrial and small-body granular environments. The open-source code CHRONO is modified and evaluated first with a series of simple two-body-collision tests, and then, with a set of piling and tumbler tests. In the piling tests, we vary the coefficient of rolling friction to calibrate the simulations against experiments with 1 mm glass beads. Then, we use the friction coefficient to model the flow of 1 mm glass beads in a rotating drum, using a drum configuration from a previous experimental study. We measure the dynamic angle of repose, the flowing layer thickness, and the flowing layer velocity for tests with different particle sizes, contact force models, coefficients of rolling friction, cohesion levels, drum rotation speeds, and gravity levels. The tests show that the same flow patterns can be observed at the Earth and reduced-gravity levels if the drum rotation speed and the gravity level are set according to the dimensionless parameter known as the Froude number. CHRONO is successfully validated against known flow behaviours at different gravity and cohesion levels, and will be used to study small-body regolith dynamics in future works.
    ISSN
    0035-8711
    EISSN
    1365-2966
    DOI
    10.1093/mnras/staa2454
    Version
    Final published version
    Sponsors
    California Institute of Technology
    ae974a485f413a2113503eed53cd6c53
    10.1093/mnras/staa2454
    Scopus Count
    Collections
    UA Faculty Publications

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