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Numerical Study of the Flow and Thermomagnetic Convection Heat Transfer of a Power Law Non-Newtonian Ferrofluid within a Circular Cavity with a Permanent Magnet

Author

Listed:
  • Nidhal Ben Khedher

    (Department of Mechanical Engineering, College of Engineering, University of Ha’il, Ha’il 81451, Saudi Arabia
    Laboratory of Thermal and Energetic Systems Studies (LESTE), National School of Engineering of Monastir, University of Monastir, Monastir 5000, Tunisia)

  • Mohammad Shahabadi

    (School of Aerospace and Mechanical Engineering, University of Oklahoma, Norman, OK 73019, USA)

  • Abed Saif Alghawli

    (Computer Science Department, Prince Sattam Bin Abdulaziz University, AL-Aflaj 11912, Saudi Arabia)

  • Christopher Neil Hulme

    (Department of Materials Science and Engineering, KTH Royal Institute of Technology, Brinellvägen 23, SE-100 44 Stockholm, Sweden)

  • Seyed Abdollah Mansouri Mehryan

    (Young Researchers and Elite Club, Yasooj Branch, Islamic Azad University, Yasooj 7591493686, Iran)

Abstract

The aim of this study is to analyze the thermo-magnetic-gravitational convection of a non-Newtonian power law ferrofluid within a circular cavity. The ferrofluid is exposed to the magnetic field of a permanent magnet. The finite element method is employed to solve the non-dimensional controlling equations. A grid sensitivity analysis and the validation of the used method are conducted. The effect of alterable parameters, including the power law index, 0.7 ≤ n ≤ 1.3, gravitational Rayleigh number, 10 4 ≤ Ra T ≤ 10 6 , magnetic Rayleigh number, 10 5 ≤ Ra M ≤ 10 8 , the location of the hot and cold surfaces, 0 ≤ λ ≤ π/2, and the length of the magnet normalized with respect to the diameter of the cavity, 0.1 ≤ L ≤ 0.65, on the flow and heat transfer characteristics are explored. The results show that the heat transfer rate increases at the end of both arcs compared to the central region because of buoyancy effects, and it is greater close to the hot arc. The location of the arcs does not affect the heat transfer rate considerably. An increase in the magnetic Rayleigh number contributes to stronger circulation of the flow inside and higher heat transfer. When the Kelvin force is the only one imposed on the flow, it enhances the heat transfer for magnets of length 0.2 ≤ L ≤ 0.3.

Suggested Citation

  • Nidhal Ben Khedher & Mohammad Shahabadi & Abed Saif Alghawli & Christopher Neil Hulme & Seyed Abdollah Mansouri Mehryan, 2022. "Numerical Study of the Flow and Thermomagnetic Convection Heat Transfer of a Power Law Non-Newtonian Ferrofluid within a Circular Cavity with a Permanent Magnet," Mathematics, MDPI, vol. 10(15), pages 1-16, July.
  • Handle: RePEc:gam:jmathe:v:10:y:2022:i:15:p:2612-:d:872245
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    References listed on IDEAS

    as
    1. Wu, Shenyi & Rincon Ortiz, Camilo, 2020. "Experimental investigation of the effect of magnetic field on vapour absorption with LiBr–H2O nanofluid," Energy, Elsevier, vol. 193(C).
    2. Nidhal Ben Khedher & Mikhail Sheremet & Abed Saif Alghawli & Abdullah Mohamed & Seyed Abdollah Mansouri Mehryan, 2022. "Effect of Non-Identical Magnetic Fields on Thermomagnetic Convective Flow of a Nanoliquid Using Buongiorno’s Model," Mathematics, MDPI, vol. 10(8), pages 1-19, April.
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