Flow and heat transfer of MHD non-Newtonian power-law fluids due to rotating disk

In flows over rotating disk, substantial additional flow phenomena arise due to the rotational forces or due to the nature of the three-dimensional boundary layer flows. The resulting flow characteristics can be very complex and almost every rotating system reveals novel and unexpected flow characte...

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Bibliographic Details
Published in:Journal of Physics: Conference Series
Main Author: Rosli N.D.K.; Kechil S.A.
Format: Conference paper
Language:English
Published: Institute of Physics Publishing 2019
Online Access:https://www.scopus.com/inward/record.uri?eid=2-s2.0-85076117128&doi=10.1088%2f1742-6596%2f1366%2f1%2f012043&partnerID=40&md5=45c84bb54d5d8f5f99fdd832aee1e0fd