Entropy Generation and Natural Convection of CuO-Water Nanofluid in C-Shaped Cavity under Magnetic Field
Abstract
:1. Introduction
2. Problem Description and Mathematical Modeling
Physical properties | Fluid phase | CuO |
---|---|---|
Cp (j/kg·K) | 4179 | 540 |
ρ (kg/m3) | 997.1 | 6500 |
Pr | 6.2 | – |
0.613 | 18 | |
() | 0.05 |
3. Numerical Solution and Grid Dependency Test
Grid points | ||||||
---|---|---|---|---|---|---|
AR = 0.1 | Ra = 1000 | 0.6884 | 0.6771 | 0.6333 | 0.6328 | 0.6328 |
Ra = 15,000 | 0.6851 | 0.6674 | 0.6617 | 0.6605 | 0.6604 | |
AR = 0.7 | Ra = 1000 | 5.2215 | 5.2069 | 5.2018 | 5.2008 | 5.2007 |
Ra = 15,000 | 5.2433 | 5.2163 | 5.2052 | 5.2026 | 5.2024 |
4. Results and Discussion
4.1. Effect of Raylirgh Number
4.2. Effect of Hartman Number
4.3. Effect of the Aspect Ratio
5. Conclusions
- (1)
- The addition of nanoparticles enhances the convective heat transfer inside the C-shaped cavity at all Rayleigh numbers, whereas the entropy generation increases with increasing the volume fraction of the nanoparticles. This increase becomes fast at higher Rayleigh number.
- (2)
- The average Nusselt number increases considerably when the hot and cold walls become narrower, i.e., at higher aspect ratio.
- (3)
- The nanofluid utilization becomes more pronounced at lower aspect ratio.
- (4)
- The applied magnetic field is an inactive process at lower Rayleigh number.
- (5)
- The entropy generation rate decreases rapidly with the applied magnetic field.
- (6)
- A threshold value of Hartman number equal to 30 can give the best thermal performance in the C-shaped cavity.
Acknowledgments
Author Contributions
Conflicts of Interest
Nomenclature
B0 | Magnetic field strength, T | Greek symbols | |
Specific heat, J·kg−1·K−1 | Thermal diffusivity, m2·s−1 | ||
Gravitational acceleration, m·s2 | Thermal expansion coefficient, K−1 | ||
Length of heat source, m | ε | performance criterion () | |
Hartmann number, | Solid volume fraction | ||
k | Thermal conductivity, W·m−1·K−1 | Effective electrical conductivity, μ·S/cm | |
Length of cavity, m | Boltzmann constant, J·K−1 | ||
Local Nusselt number | Dimensionless temperature, | ||
Num | Average Nusselt number of heat source | Dynamic viscosity, N·S·m−2 | |
Fluid pressure, Pa | Kinematic viscosity, m2·s−1 | ||
Dimensionless pressure, | Density, kg·m3 | ||
Prandtl number, νf/αf | Subscripts | ||
Temperature, K | Cold | ||
Tc | Cold wall temperature, K | Pure fluid | |
Hot wall temperature, K | hot wall | ||
Velocity components in x, y directions, m·s−1 | Average | ||
Dimensionless Velocity components, | Nanofluid | ||
Cartesian coordinates, m | Nanoparticle | ||
X,Y | Dimensionless coordinates, (x,y)/L |
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Chamkha, A.; Ismael, M.; Kasaeipoor, A.; Armaghani, T. Entropy Generation and Natural Convection of CuO-Water Nanofluid in C-Shaped Cavity under Magnetic Field. Entropy 2016, 18, 50. https://doi.org/10.3390/e18020050
Chamkha A, Ismael M, Kasaeipoor A, Armaghani T. Entropy Generation and Natural Convection of CuO-Water Nanofluid in C-Shaped Cavity under Magnetic Field. Entropy. 2016; 18(2):50. https://doi.org/10.3390/e18020050
Chicago/Turabian StyleChamkha, Ali, Muneer Ismael, Abbas Kasaeipoor, and Taher Armaghani. 2016. "Entropy Generation and Natural Convection of CuO-Water Nanofluid in C-Shaped Cavity under Magnetic Field" Entropy 18, no. 2: 50. https://doi.org/10.3390/e18020050
APA StyleChamkha, A., Ismael, M., Kasaeipoor, A., & Armaghani, T. (2016). Entropy Generation and Natural Convection of CuO-Water Nanofluid in C-Shaped Cavity under Magnetic Field. Entropy, 18(2), 50. https://doi.org/10.3390/e18020050