Abstract
The effect of magnetic field on natural convection heat transfer in an L-shaped enclosure filled with a non-Newtonian fluid is investigated numerically. The governing equations are solved by finite-volume method using the SIMPLE algorithm. The power-law rheological model is used to characterize the non-Newtonian fluid behavior. It is revealed that heat transfer rate decreases for shear-thinning fluids (of power-law index, n < 1) and increases for shear-thickening fluids (n > 1) in comparison with the Newtonian ones. Thermal behavior of shear-thinning and shear-thickening fluids is similar to that of Newtonian fluids for the angle of enclosure α < 60° and α > 60°, respectively.
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Abbreviations
- AR:
-
Aspect ratio
- B o :
-
Magnetic induction (T)
- g :
-
Gravitational acceleration (m s−2)
- Ha:
-
Hartmann number
- K :
-
Thermal conductivity (W m−1 K−1)
- L :
-
Specific length (m)
- n :
-
Power-law index
- Nu:
-
Local Nusselt number
- P :
-
Pressure (Pa)
- Pr:
-
Prandtl number
- Ra:
-
Rayleigh number
- Re:
-
Reynolds number
- T :
-
Wall temperature (K)
- u :
-
Velocity in x-direction (m s−1)
- v :
-
Velocity in y-direction (m s−1)
- U :
-
Dimensionless velocity in x-direction
- V :
-
Dimensionless velocity in y-direction
- x :
-
Distance along x-coordinate
- y :
-
Distance along y-coordinate
- β :
-
Thermal expansion coefficient (k−1)
- μ :
-
Dynamic viscosity (kg m−1 s−1)
- ρ :
-
Density (kg m−3)
- θ :
-
Dimensionless temperature
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Jahanbakhshi, A., Nadooshan, A.A. & Bayareh, M. Magnetic field effects on natural convection flow of a non-Newtonian fluid in an L-shaped enclosure. J Therm Anal Calorim 133, 1407–1416 (2018). https://doi.org/10.1007/s10973-018-7219-6
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DOI: https://doi.org/10.1007/s10973-018-7219-6