Show simple item record

dc.contributor.authorBattista, Nicholas
dc.contributor.authorMiller, Laura
dc.date.accessioned2022-12-05T21:16:31Z
dc.date.available2022-12-05T21:16:31Z
dc.date.issued2013-11
dc.identifier.citationBattista, N. A., & Miller, L. (2013). Pulsatile flow through idealized trabeculae. Bulletin of the American Physical Society, 58(18).en_US
dc.identifier.urihttp://meetings.aps.org/link/BAPS.2013.DFD.A16.7
dc.identifier.urihttp://dr.tcnj.edu/handle/2900/4077
dc.descriptionDepartment of Mathematics and Statisticsen_US
dc.description.abstractTrabeculae begin to form in the human developing heart for Reynolds numbers on the order of 10. Other hearts, such as the squid heart, have trabeculae for Re on the order of 10 and larger. The effect of trabeculae on the flow in this range of Re is not well understood. In this study, computational fluid dynamics is used to quantify the effects of Reynolds number and idealized trabeculae height on the resulting flows. An adaptive and parallelized version of the immersed boundary method (IBAMR) is used to solve the fluid-structure interaction problem. We see the formation of vortices depends upon Re and trabeculae height. We then explore how the periodicity of the flow effects vortex formation and shear patterns. This is important because it is thought that these dynamic processes are important to the generation of shear at the endothelial surface layer and strains at the epithelial layer, which will aid in proper development and functionality.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsFile not available for download due to copyright restrictionsen_US
dc.titlePulsatile flow through idealized trabeculaeen_US
dc.typeArticleen_US
dc.typeTexten_US
prism.publicationNameBulletin of the American Physical Societyen_US
prism.volume58
prism.issueIdentifier18


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record