Collisions of Porous Clusters: A Granular-mechanics Study

Autores
Ringl, Christian; Bringa, Eduardo Marcial; Bertoldi, Dalía Surena; Urbassek, Herbert M.
Año de publicación
2012
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The collision of granular clusters can result in a number of complex outcomes from sticking to partial or full destruction of the clusters. These outcomes will contribute to the size distribution of dust aggregates, changing their optical properties and their capability to contribute to solid-state astrochemistry. We study the collision of two clusters of equal size, formed by approximately 7000 sub-μm grains each, with a mass and velocity range that is difficult to sample in experiments. We obtain the outcome of the collision: compaction, fragmentation, and size distribution of ejecta, and type of outcome, as a function of velocity and impact parameter. We compare our results to other models and simulations, at both atomistic and continuum scales, and find some agreement together with some discrepancies. We also study collision-induced compaction as a function of cluster size, up to sizes of N = 250,000, and find that for large clusters considerably higher compactions result at higher velocities.
Fil: Ringl, Christian. University of Kaiserslautern; Alemania
Fil: Bringa, Eduardo Marcial. 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
Fil: Bertoldi, Dalía Surena. 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
Fil: Urbassek, Herbert M.. University of Kaiserslautern; Alemania
Materia
Statistical methods
Planets and satellites
Animations
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/272809

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spelling Collisions of Porous Clusters: A Granular-mechanics StudyRingl, ChristianBringa, Eduardo MarcialBertoldi, Dalía SurenaUrbassek, Herbert M.Statistical methodsPlanets and satellitesAnimationshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The collision of granular clusters can result in a number of complex outcomes from sticking to partial or full destruction of the clusters. These outcomes will contribute to the size distribution of dust aggregates, changing their optical properties and their capability to contribute to solid-state astrochemistry. We study the collision of two clusters of equal size, formed by approximately 7000 sub-μm grains each, with a mass and velocity range that is difficult to sample in experiments. We obtain the outcome of the collision: compaction, fragmentation, and size distribution of ejecta, and type of outcome, as a function of velocity and impact parameter. We compare our results to other models and simulations, at both atomistic and continuum scales, and find some agreement together with some discrepancies. We also study collision-induced compaction as a function of cluster size, up to sizes of N = 250,000, and find that for large clusters considerably higher compactions result at higher velocities.Fil: Ringl, Christian. University of Kaiserslautern; AlemaniaFil: Bringa, Eduardo Marcial. 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; ArgentinaFil: Bertoldi, Dalía Surena. 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; ArgentinaFil: Urbassek, Herbert M.. University of Kaiserslautern; AlemaniaIOP Publishing2012-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/272809Ringl, Christian; Bringa, Eduardo Marcial; Bertoldi, Dalía Surena; Urbassek, Herbert M.; Collisions of Porous Clusters: A Granular-mechanics Study; IOP Publishing; Astrophysical Journal; 752; 2; 6-2012; 1-130004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-637X/752/2/151info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/752/2/151info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:26:52Zoai:ri.conicet.gov.ar:11336/272809instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-15 14:26:52.989CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Collisions of Porous Clusters: A Granular-mechanics Study
title Collisions of Porous Clusters: A Granular-mechanics Study
spellingShingle Collisions of Porous Clusters: A Granular-mechanics Study
Ringl, Christian
Statistical methods
Planets and satellites
Animations
title_short Collisions of Porous Clusters: A Granular-mechanics Study
title_full Collisions of Porous Clusters: A Granular-mechanics Study
title_fullStr Collisions of Porous Clusters: A Granular-mechanics Study
title_full_unstemmed Collisions of Porous Clusters: A Granular-mechanics Study
title_sort Collisions of Porous Clusters: A Granular-mechanics Study
dc.creator.none.fl_str_mv Ringl, Christian
Bringa, Eduardo Marcial
Bertoldi, Dalía Surena
Urbassek, Herbert M.
author Ringl, Christian
author_facet Ringl, Christian
Bringa, Eduardo Marcial
Bertoldi, Dalía Surena
Urbassek, Herbert M.
author_role author
author2 Bringa, Eduardo Marcial
Bertoldi, Dalía Surena
Urbassek, Herbert M.
author2_role author
author
author
dc.subject.none.fl_str_mv Statistical methods
Planets and satellites
Animations
topic Statistical methods
Planets and satellites
Animations
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The collision of granular clusters can result in a number of complex outcomes from sticking to partial or full destruction of the clusters. These outcomes will contribute to the size distribution of dust aggregates, changing their optical properties and their capability to contribute to solid-state astrochemistry. We study the collision of two clusters of equal size, formed by approximately 7000 sub-μm grains each, with a mass and velocity range that is difficult to sample in experiments. We obtain the outcome of the collision: compaction, fragmentation, and size distribution of ejecta, and type of outcome, as a function of velocity and impact parameter. We compare our results to other models and simulations, at both atomistic and continuum scales, and find some agreement together with some discrepancies. We also study collision-induced compaction as a function of cluster size, up to sizes of N = 250,000, and find that for large clusters considerably higher compactions result at higher velocities.
Fil: Ringl, Christian. University of Kaiserslautern; Alemania
Fil: Bringa, Eduardo Marcial. 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
Fil: Bertoldi, Dalía Surena. 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
Fil: Urbassek, Herbert M.. University of Kaiserslautern; Alemania
description The collision of granular clusters can result in a number of complex outcomes from sticking to partial or full destruction of the clusters. These outcomes will contribute to the size distribution of dust aggregates, changing their optical properties and their capability to contribute to solid-state astrochemistry. We study the collision of two clusters of equal size, formed by approximately 7000 sub-μm grains each, with a mass and velocity range that is difficult to sample in experiments. We obtain the outcome of the collision: compaction, fragmentation, and size distribution of ejecta, and type of outcome, as a function of velocity and impact parameter. We compare our results to other models and simulations, at both atomistic and continuum scales, and find some agreement together with some discrepancies. We also study collision-induced compaction as a function of cluster size, up to sizes of N = 250,000, and find that for large clusters considerably higher compactions result at higher velocities.
publishDate 2012
dc.date.none.fl_str_mv 2012-06
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/272809
Ringl, Christian; Bringa, Eduardo Marcial; Bertoldi, Dalía Surena; Urbassek, Herbert M.; Collisions of Porous Clusters: A Granular-mechanics Study; IOP Publishing; Astrophysical Journal; 752; 2; 6-2012; 1-13
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/272809
identifier_str_mv Ringl, Christian; Bringa, Eduardo Marcial; Bertoldi, Dalía Surena; Urbassek, Herbert M.; Collisions of Porous Clusters: A Granular-mechanics Study; IOP Publishing; Astrophysical Journal; 752; 2; 6-2012; 1-13
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/0004-637X/752/2/151
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/752/2/151
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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