Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/184
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dc.contributor.authorShahzad, Faisal-
dc.contributor.authorJamshed, Wasim-
dc.contributor.authorSafdar, Rabia-
dc.contributor.authorHussain, Syed M.-
dc.contributor.authorDhange, Mallinath-
dc.date.accessioned2022-06-01T11:13:39Z-
dc.date.available2022-06-01T11:13:39Z-
dc.date.issued2022-03-
dc.identifier.urihttp://hdl.handle.net/123456789/184-
dc.description.abstractThe mathematical modeling of hybrid nano- fluid flow and heat transfer with entropy generation toward parabolic trough surface collector (PTSC) inside the solar-powered ship (SPS) is performed. The mathe- matical model used non-Newtonian Oldroyd-B model amidst a constant inclined magnetic field influence is being considered. The mathematical model is then reduced by adopting appropriate similarity transformation into a higher-order nonlinear differential equations system. The reduced model is computed using the well-known tech- nique called the Keller Box scheme. Physical parameters effectiveness, for instance, thermal radiation, viscous dissi- pation, hybrid nanoparticles, and Joule heating, is displayed in graphs. The silver-ethylene glycol (Ag-EG) characteristic performance outperformed the silver-magnetite-ethylene glycol (Ag-Fe 3 O 4 /EG). The maximum efficiency of Ag-EG is about 26.3%, while the minimum is at least 5.6%. Keywords: PTSC, solar-powered ship, angle of inclina- tion, Oldroyd B-hybrid nanofluid, entropy formation, MHD, Keller box methoden_US
dc.language.isoen_USen_US
dc.publisherDe Gruyteren_US
dc.relation.ispartofseries2015–2037;-
dc.subjectPTSC, solar-powered ship, angle of inclina- tion, Oldroyd B-hybrid nanofluid, entropy formation, MHD, Keller box methoden_US
dc.titleThermal analysis characterisation of solar- powered ship using Oldroyd hybrid nanofluids in parabolic trough solar collector: An optimal thermal applicationen_US
dc.typeArticleen_US
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