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Welcome to the Bahria University DSpace digital repository. DSpace is a digital service that collects, preserves, and distributes digital material. Repositories are important tools for preserving an organization's legacy; they facilitate digital preservation and scholarly communication.
| dc.contributor.author | Hafsa Bint E Arlf, 01-248202-004 | |
| dc.date.accessioned | 2022-12-22T08:03:24Z | |
| dc.date.available | 2022-12-22T08:03:24Z | |
| dc.date.issued | 2022 | |
| dc.identifier.uri | http://hdl.handle.net/123456789/14516 | |
| dc.description | Supervised by Dr. Muhammad Ramzan | en_US |
| dc.description.abstract | This steady discusses the flow of Holroyd-B nanofluid amidst two rotating disks with the inclusion of gyrostatic microorganisms. The stability of the nanofluid flow is strengthened by embedding the impact of the gyrostatic microorganisms. The Buongiorno model is adopted for the nanofluid flow. The Hall current and Ion slip impact are considered owing to the strong magnetic field taken perpendicular to the both disks. The envisioned model is tackled numerically and graphs of arising parameters are plotted against associated profiles. The physical quantities of interest are also investigated | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Computer Sciences | en_US |
| dc.relation.ispartofseries | MS (DS);T-01897 | |
| dc.subject | Gyrostatic Microorganisms | en_US |
| dc.subject | Nanofluid Flow | en_US |
| dc.title | Hall Current and Ion Slip Impact on a Oldroyd-b Nanofluid Flow Driven by two Concentric Rotating Disks with Cattaneo-Christov Heat Flux | en_US |
| dc.type | MS Thesis | en_US |
