Numerical simulation of mass and heat transport phenomena of hydromagnetic flow of Casson fluid with sinusoidal boundary conditions

bracu.type.groupResearch Publications
datacite.rightsOpen Access
dc.contributor.authorIslam M.R.
dc.contributor.authorReza-E-Rabbi S.
dc.contributor.authorYousuf Ali M.
dc.contributor.authorRasel, Md. Mehedi Hasan
dc.contributor.authorAhmmed S.F.
dc.contributor.departmentDepartment of Mathematics and Natural Sciences
dc.date.accessioned2026-10-10T06:37:12Z
dc.date.available2026-10-10T06:37:12Z
dc.date.issued2023-11-01
dc.description.abstractA magnetic field might interact with its surroundings, influencing chemical and physical processes in materials processing, heat exchangers, and other scientific study. Therefore, a computational study of non-Newtonian (Casson) free convective MHD unsteady fluid flow has been highlighted in this article with mass and heat transit property through a vertical infinite porous plate. A sinusoidal boundary conditions as well as chemical reaction and thermal radiation have been considered. Using a collection of nondimensional variables, the flow related equations are also turned into nondimensional form. The EFDM algorithm is employed in order to arrive at a numerical solution via Compaq Visual Fortran. The reliability of the numerical solution has been confirmed using stability testing and convergence analysis. The whole system is convergent when the values of Prandtl number and Lewis number are greater than or equals to 0.075 and 0.025, respectively. A visual depiction of the impact of the pertinent factors on dimensionless velocity, temperature, and concentration profiles are displayed through graphical representation as well as with tabular representation. It has been inspected that when the magnetic component is regarded, it greatly affects the heat transfer factors of Casson nanofluid and the heat also rises when Eckert number, heat source and radiation parameter accelerate. It is also found that the Sherwood number is increased as the impact of chemical reaction parameter and the Lewis number, also the skin friction is decreased as the influence of porosity term got accelerated. The comparison of the current findings with the data that were previously published serves as the final stage in validating the present study.
dc.description.versionPublished
dc.format.extent26 pages
dc.identifier.citationIslam, M. R., Reza-E-Rabbi, S., Yousuf Ali, M., Rasel, M. M. H., & Ahmmed, S. F. (2023). Numerical simulation of mass and heat transport phenomena of hydromagnetic flow of Casson fluid with sinusoidal boundary conditions. Engineering Reports, 5(11), Article e12659. https://doi.org/10.1002/eng2.12659
dc.identifier.doi10.1002/eng2.12659
dc.identifier.issn25778196
dc.identifier.other2-s2.0-85152652632
dc.identifier.urihttps://hdl.handle.net/10361/30578
dc.language.isoen_US
dc.publisherJohn Wiley and Sons Inc.
dc.relation.hasversion10.1002/eng2.12659
dc.relation.ispartofEngineering Reports
dc.relation.ispartofseriesEngineering Reports
dc.relation.journalEngineering Reports
dc.relation.urihttps://onlinelibrary.wiley.com/doi/10.1002/eng2.12659
dc.subjectMHD
dc.subjectNanofluid
dc.subjectChemical reaction
dc.subjectSinusoidal boundary conditions
dc.subjectThermal radiation
dc.subjectCasson fluids
dc.subjectMagnetohydrodynamics
dc.subject.lcshFluid dynamics--Mathematical models.
dc.subject.lcshHeat--Transmission.
dc.subject.lcshMass transfer.
dc.subject.lcshMagnetohydrodynamics--Mathematical models.
dc.subject.lcshNon-Newtonian fluids--Mathematical models.
dc.titleNumerical simulation of mass and heat transport phenomena of hydromagnetic flow of Casson fluid with sinusoidal boundary conditions
dc.typeArticle
oaire.citation.issue11
oaire.citation.volume5
person.affiliation.namePabna University of Science and Technology
person.affiliation.nameKhulna University
person.affiliation.nameKhulna University
person.affiliation.nameBRAC University
person.affiliation.nameKhulna University
person.identifier.orcid0000-0002-4079-7507
person.identifier.scopus-author-id59518411300
person.identifier.scopus-author-id57204535903
person.identifier.scopus-author-id57693651800
person.identifier.scopus-author-id58107885300
person.identifier.scopus-author-id55909594400

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