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dc.contributor.author
Bandyopadhyay, Rahul
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Planes, María Belén
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Millán, Emmanuel Nicolás
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Bringa, Eduardo Marcial
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Urbassek, Herbert M.
dc.date.available
2024-03-14T10:52:08Z
dc.date.issued
2023-09
dc.identifier.citation
Bandyopadhyay, Rahul; Planes, María Belén; Millán, Emmanuel Nicolás; Bringa, Eduardo Marcial; Urbassek, Herbert M.; Impact of internal structure on aggregate collisions; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 526; 1; 9-2023; 523-533
dc.identifier.issn
0035-8711
dc.identifier.uri
http://hdl.handle.net/11336/230441
dc.description.abstract
Granular-mechanics simulations are used to study collisions between granular aggregates. We compare the collision outcomes for three different types of aggregate: (i) aggregates constructed by a ballistic particle-cluster aggregation (BPCA) process, and two homogeneous spherical aggregates which differ by their grain coordination. All aggregates contain the same number of grains and (central) filling factor. We find that BPCA aggregates have a slightly decreased growth velocity for central impacts. After scaling the collision velocities to the growth velocity for central impact and the impact parameter to the gyration radius, our collision results show a remarkable degree of agreement for the aggregates studied. Also, the collision-induced compaction as well as the size of fluctuations during the collision process are identical for all aggregate types. Even at glancing collisions, the larger extension and rough surface of BPCA aggregates do not cause major changes as compared to homogeneous aggregates with a well-defined and smooth surface. However, monomer ejection during the collision is enhanced for BPCA aggregates. This study thus shows that details of the internal aggregate structure are of little importance in collisions of granular aggregates, except for grain ejection.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Oxford University Press
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
planets and satellites: formation
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protoplanetary disks
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methods: numerical
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Otras Ciencias Físicas
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Impact of internal structure on aggregate collisions
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2024-03-13T14:24:48Z
dc.identifier.eissn
1365-2966
dc.journal.volume
526
dc.journal.number
1
dc.journal.pagination
523-533
dc.journal.pais
Reino Unido
dc.description.fil
Fil: Bandyopadhyay, Rahul. Universitat Kaiserslautern; Alemania
dc.description.fil
Fil: Planes, María Belén. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
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Fil: Millán, Emmanuel Nicolás. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
dc.description.fil
Fil: Bringa, Eduardo Marcial. Universidad Mayor.; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mendoza. Instituto Interdisciplinario de Ciencias Básicas. - Universidad Nacional de Cuyo. Instituto Interdisciplinario de Ciencias Básicas; Argentina
dc.description.fil
Fil: Urbassek, Herbert M.. Universitat Kaiserslautern; Alemania
dc.journal.title
Monthly Notices of the Royal Astronomical Society
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stad2828/7276622
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stad2828
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