Phase diagram for inertial granular flows

Flows of hard granular materials depend strongly on the interparticle friction coefficient μ_{p} and on the inertial number I, which characterizes proximity to the jamming transition where flow stops. Guided by numerical simulations, we derive the phase diagram of dense inertial flow of spherical pa...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review. E 2016-07, Vol.94 (1-1), p.012904-012904, Article 012904
Hauptverfasser: DeGiuli, E, McElwaine, J N, Wyart, M
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 012904
container_issue 1-1
container_start_page 012904
container_title Physical review. E
container_volume 94
creator DeGiuli, E
McElwaine, J N
Wyart, M
description Flows of hard granular materials depend strongly on the interparticle friction coefficient μ_{p} and on the inertial number I, which characterizes proximity to the jamming transition where flow stops. Guided by numerical simulations, we derive the phase diagram of dense inertial flow of spherical particles, finding three regimes for 10^{-4}≲I≲10^{-1}: frictionless, frictional sliding, and rolling. These are distinguished by the dominant means of energy dissipation, changing from collisional to sliding friction, and back to collisional, as μ_{p} increases from zero at constant I. The three regimes differ in their kinetics and rheology; in particular, the velocity fluctuations and the stress ratio both display nonmonotonic behavior with μ_{p}, corresponding to transitions between the three regimes of flow. We rationalize the phase boundaries between these regimes, show that energy balance yields scaling relations between microscopic properties in each of them, and derive the strain scale at which particles lose memory of their velocity. For the frictional sliding regime most relevant experimentally, we find for I≥10^{-2.5} that the growth of the macroscopic friction μ(I) with I is induced by an increase of collisional dissipation. This implies in that range that μ(I)-μ(0)∼I^{1-2b}, where b≈0.2 is an exponent that characterizes both the dimensionless velocity fluctuations L∼I^{-b} and the density of sliding contacts χ∼I^{b}.
doi_str_mv 10.1103/PhysRevE.94.012904
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1815976839</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1815976839</sourcerecordid><originalsourceid>FETCH-LOGICAL-c347t-cc17c465b9bc591cfb807ca6731257a681d21470299e38f1cf1209076b1047e63</originalsourceid><addsrcrecordid>eNo9kE1Lw0AQhhdRbKn9Ax4kRz2kzuxn9iilfkDBInpeNpuNjSRN3U2U_nsj_TjNMDzvy_AQco0wQwR2v1rv4pv_Wcw0nwFSDfyMjClXkAIIdn7auRiRaYxfAIAStEJ6SUZUCSUosDG5W61t9ElR2c9gm6RsQ1JtfOgqWyfDZdPXNiRl3f7GK3JR2jr66WFOyMfj4n3-nC5fn17mD8vUMa661DlUjkuR69wJja7MM1DOSsWQCmVlhgXF4TWqtWdZOQBIQYOSOQJXXrIJud33bkP73fvYmaaKzte13fi2jwYzFFrJjOkBpXvUhTbG4EuzDVVjw84gmH9L5mjJaG72lobQzaG_zxtfnCJHJ-wPIFVh9w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1815976839</pqid></control><display><type>article</type><title>Phase diagram for inertial granular flows</title><source>American Physical Society Journals</source><creator>DeGiuli, E ; McElwaine, J N ; Wyart, M</creator><creatorcontrib>DeGiuli, E ; McElwaine, J N ; Wyart, M</creatorcontrib><description>Flows of hard granular materials depend strongly on the interparticle friction coefficient μ_{p} and on the inertial number I, which characterizes proximity to the jamming transition where flow stops. Guided by numerical simulations, we derive the phase diagram of dense inertial flow of spherical particles, finding three regimes for 10^{-4}≲I≲10^{-1}: frictionless, frictional sliding, and rolling. These are distinguished by the dominant means of energy dissipation, changing from collisional to sliding friction, and back to collisional, as μ_{p} increases from zero at constant I. The three regimes differ in their kinetics and rheology; in particular, the velocity fluctuations and the stress ratio both display nonmonotonic behavior with μ_{p}, corresponding to transitions between the three regimes of flow. We rationalize the phase boundaries between these regimes, show that energy balance yields scaling relations between microscopic properties in each of them, and derive the strain scale at which particles lose memory of their velocity. For the frictional sliding regime most relevant experimentally, we find for I≥10^{-2.5} that the growth of the macroscopic friction μ(I) with I is induced by an increase of collisional dissipation. This implies in that range that μ(I)-μ(0)∼I^{1-2b}, where b≈0.2 is an exponent that characterizes both the dimensionless velocity fluctuations L∼I^{-b} and the density of sliding contacts χ∼I^{b}.</description><identifier>ISSN: 2470-0045</identifier><identifier>EISSN: 2470-0053</identifier><identifier>DOI: 10.1103/PhysRevE.94.012904</identifier><identifier>PMID: 27575203</identifier><language>eng</language><publisher>United States</publisher><ispartof>Physical review. E, 2016-07, Vol.94 (1-1), p.012904-012904, Article 012904</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c347t-cc17c465b9bc591cfb807ca6731257a681d21470299e38f1cf1209076b1047e63</citedby><cites>FETCH-LOGICAL-c347t-cc17c465b9bc591cfb807ca6731257a681d21470299e38f1cf1209076b1047e63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,2874,2875,27922,27923</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/27575203$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>DeGiuli, E</creatorcontrib><creatorcontrib>McElwaine, J N</creatorcontrib><creatorcontrib>Wyart, M</creatorcontrib><title>Phase diagram for inertial granular flows</title><title>Physical review. E</title><addtitle>Phys Rev E</addtitle><description>Flows of hard granular materials depend strongly on the interparticle friction coefficient μ_{p} and on the inertial number I, which characterizes proximity to the jamming transition where flow stops. Guided by numerical simulations, we derive the phase diagram of dense inertial flow of spherical particles, finding three regimes for 10^{-4}≲I≲10^{-1}: frictionless, frictional sliding, and rolling. These are distinguished by the dominant means of energy dissipation, changing from collisional to sliding friction, and back to collisional, as μ_{p} increases from zero at constant I. The three regimes differ in their kinetics and rheology; in particular, the velocity fluctuations and the stress ratio both display nonmonotonic behavior with μ_{p}, corresponding to transitions between the three regimes of flow. We rationalize the phase boundaries between these regimes, show that energy balance yields scaling relations between microscopic properties in each of them, and derive the strain scale at which particles lose memory of their velocity. For the frictional sliding regime most relevant experimentally, we find for I≥10^{-2.5} that the growth of the macroscopic friction μ(I) with I is induced by an increase of collisional dissipation. This implies in that range that μ(I)-μ(0)∼I^{1-2b}, where b≈0.2 is an exponent that characterizes both the dimensionless velocity fluctuations L∼I^{-b} and the density of sliding contacts χ∼I^{b}.</description><issn>2470-0045</issn><issn>2470-0053</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNo9kE1Lw0AQhhdRbKn9Ax4kRz2kzuxn9iilfkDBInpeNpuNjSRN3U2U_nsj_TjNMDzvy_AQco0wQwR2v1rv4pv_Wcw0nwFSDfyMjClXkAIIdn7auRiRaYxfAIAStEJ6SUZUCSUosDG5W61t9ElR2c9gm6RsQ1JtfOgqWyfDZdPXNiRl3f7GK3JR2jr66WFOyMfj4n3-nC5fn17mD8vUMa661DlUjkuR69wJja7MM1DOSsWQCmVlhgXF4TWqtWdZOQBIQYOSOQJXXrIJud33bkP73fvYmaaKzte13fi2jwYzFFrJjOkBpXvUhTbG4EuzDVVjw84gmH9L5mjJaG72lobQzaG_zxtfnCJHJ-wPIFVh9w</recordid><startdate>201607</startdate><enddate>201607</enddate><creator>DeGiuli, E</creator><creator>McElwaine, J N</creator><creator>Wyart, M</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>201607</creationdate><title>Phase diagram for inertial granular flows</title><author>DeGiuli, E ; McElwaine, J N ; Wyart, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c347t-cc17c465b9bc591cfb807ca6731257a681d21470299e38f1cf1209076b1047e63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>DeGiuli, E</creatorcontrib><creatorcontrib>McElwaine, J N</creatorcontrib><creatorcontrib>Wyart, M</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Physical review. E</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>DeGiuli, E</au><au>McElwaine, J N</au><au>Wyart, M</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Phase diagram for inertial granular flows</atitle><jtitle>Physical review. E</jtitle><addtitle>Phys Rev E</addtitle><date>2016-07</date><risdate>2016</risdate><volume>94</volume><issue>1-1</issue><spage>012904</spage><epage>012904</epage><pages>012904-012904</pages><artnum>012904</artnum><issn>2470-0045</issn><eissn>2470-0053</eissn><abstract>Flows of hard granular materials depend strongly on the interparticle friction coefficient μ_{p} and on the inertial number I, which characterizes proximity to the jamming transition where flow stops. Guided by numerical simulations, we derive the phase diagram of dense inertial flow of spherical particles, finding three regimes for 10^{-4}≲I≲10^{-1}: frictionless, frictional sliding, and rolling. These are distinguished by the dominant means of energy dissipation, changing from collisional to sliding friction, and back to collisional, as μ_{p} increases from zero at constant I. The three regimes differ in their kinetics and rheology; in particular, the velocity fluctuations and the stress ratio both display nonmonotonic behavior with μ_{p}, corresponding to transitions between the three regimes of flow. We rationalize the phase boundaries between these regimes, show that energy balance yields scaling relations between microscopic properties in each of them, and derive the strain scale at which particles lose memory of their velocity. For the frictional sliding regime most relevant experimentally, we find for I≥10^{-2.5} that the growth of the macroscopic friction μ(I) with I is induced by an increase of collisional dissipation. This implies in that range that μ(I)-μ(0)∼I^{1-2b}, where b≈0.2 is an exponent that characterizes both the dimensionless velocity fluctuations L∼I^{-b} and the density of sliding contacts χ∼I^{b}.</abstract><cop>United States</cop><pmid>27575203</pmid><doi>10.1103/PhysRevE.94.012904</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 2470-0045
ispartof Physical review. E, 2016-07, Vol.94 (1-1), p.012904-012904, Article 012904
issn 2470-0045
2470-0053
language eng
recordid cdi_proquest_miscellaneous_1815976839
source American Physical Society Journals
title Phase diagram for inertial granular flows
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-14T12%3A26%3A25IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Phase%20diagram%20for%20inertial%20granular%20flows&rft.jtitle=Physical%20review.%20E&rft.au=DeGiuli,%20E&rft.date=2016-07&rft.volume=94&rft.issue=1-1&rft.spage=012904&rft.epage=012904&rft.pages=012904-012904&rft.artnum=012904&rft.issn=2470-0045&rft.eissn=2470-0053&rft_id=info:doi/10.1103/PhysRevE.94.012904&rft_dat=%3Cproquest_cross%3E1815976839%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1815976839&rft_id=info:pmid/27575203&rfr_iscdi=true