kth.sePublications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Chaos and irreversibility of a flexible filament in periodically driven Stokes flow
Nordita SU; Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden.;Stockholm Univ, Dept Phys, S-10691 Stockholm, Sweden..
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA.ORCID iD: 0000-0001-6162-7112
2022 (English)In: Physical review. E, ISSN 2470-0045, E-ISSN 2470-0053, Vol. 106, no 2, article id 025103Article in journal (Refereed) Published
Abstract [en]

The flow of Newtonian fluid at low Reynolds number is, in general, regular and time-reversible due to absence of nonlinear effects. For example, if the fluid is sheared by its boundary motion that is subsequently reversed, then all the fluid elements return to their initial positions. Consequently, mixing in microchannels happens solely due to molecular diffusion and is very slow. Here, we show, numerically, that the introduction of a single, freely floating, flexible filament in a time-periodic linear shear flow can break reversibility and give rise to chaos due to elastic nonlinearities, if the bending rigidity of the filament is within a carefully chosen range. Within this range, not only the shape of the filament is spatiotemporally chaotic, but also the flow is an efficient mixer. Overall, we find five dynamical phases: the shape of a stiff filament is time-invariant-either straight or buckled; it undergoes a period-two bifurcation as the filament is made softer; becomes spatiotemporally chaotic for even softer filaments but, surprisingly, the chaos is suppressed if bending rigidity is decreased further.

Place, publisher, year, edition, pages
American Physical Society (APS) , 2022. Vol. 106, no 2, article id 025103
National Category
Physical Sciences Other Physics Topics
Identifiers
URN: urn:nbn:se:kth:diva-319722DOI: 10.1103/PhysRevE.106.025103ISI: 000860439400002PubMedID: 36109885Scopus ID: 2-s2.0-85137870821OAI: oai:DiVA.org:kth-319722DiVA, id: diva2:1707445
Note

QC 20221031

Available from: 2022-10-31 Created: 2022-10-31 Last updated: 2022-10-31Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full textPubMedScopus

Authority records

Mitra, Dhrubaditya

Search in DiVA

By author/editor
Mitra, Dhrubaditya
By organisation
Nordic Institute for Theoretical Physics NORDITA
In the same journal
Physical review. E
Physical SciencesOther Physics Topics

Search outside of DiVA

GoogleGoogle Scholar

doi
pubmed
urn-nbn

Altmetric score

doi
pubmed
urn-nbn
Total: 147 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf