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dc.contributor.authorSunday, Cecily
dc.contributor.authorMurdoch, Naomi
dc.contributor.authorTardivel, Simon
dc.contributor.authorSchwartz, Stephen R
dc.contributor.authorMichel, Patrick
dc.date.accessioned2021-04-28T19:00:51Z
dc.date.available2021-04-28T19:00:51Z
dc.date.issued2020-08-18
dc.identifier.citationSunday, 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.en_US
dc.identifier.issn0035-8711
dc.identifier.doi10.1093/mnras/staa2454
dc.identifier.urihttp://hdl.handle.net/10150/657952
dc.description.abstractThe 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.en_US
dc.description.sponsorshipCalifornia Institute of Technologyen_US
dc.language.isoenen_US
dc.publisherOXFORD UNIV PRESSen_US
dc.rights© 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.en_US
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectmethods: numericalen_US
dc.subjectplanets and satellites: generalen_US
dc.subjectplanets and satellites: surfacesen_US
dc.subjectsoftware: simulationsen_US
dc.subjectsoftware: developmenten_US
dc.titleValidating N-body code chrono for granular DEM simulations in reduced-gravity environmentsen_US
dc.typeArticleen_US
dc.identifier.eissn1365-2966
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben_US
dc.identifier.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYen_US
dc.description.collectioninformationThis 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.en_US
dc.eprint.versionFinal published versionen_US
dc.source.journaltitleMonthly Notices of the Royal Astronomical Society
dc.source.volume498
dc.source.issue1
dc.source.beginpage1062
dc.source.endpage1079
refterms.dateFOA2021-04-28T19:00:53Z


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