Abstract
In current challenge, the entropy generation approach is painted particularly as a powerful tool for the analysis of the brain function, in accordance with the theoretical and philosophical approach of Saint Thomas Aquinas. The present assessment is considered to look at the entropy minimization in MHD flow of a Williamson nanofluid flow past a stretchable surface under the effects of Thomson and Troian boundary condition. The flow is induced in the system because of the linear movement of stretched surface which is porous. Heat and mass transportations are the modern aspects in the flow, for this, theories of Cattaneo-Christov heat flux is used in this study. Moreover, viscous dissipation and thermal radiation impacts are taken place in the energy equation with linear expression. Additionally, the impact of heat generation or absorption with nonlinear expressions is also considered in the existing continuation which makes the study quite versatile. The finite difference strategy, for example bvp4c from Mat Lab is applied to solve the reduced ordinary differential equations. The proposed technique is more appropriate to solve the considered problem in the present analysis when compared to other previous works. From all these lines, observations are noted as due to the slip factor the velocity profile is declined and temperature distribution is improved. Because of utility of nanoparticles, Bejan number distribution is increased with the Weissenberg number and thermophoresis constant increments. From the analysis, present study is applicable in the fields of manufacturing processes and improvement in energy and heat resources.
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Abbreviations
- \(\left( {u. v} \right)\) :
-
Velocity components \(\left( {ms^{ - 1} } \right)\)
- \(\left( {x,y} \right)\) :
-
Cartesian coordinates \(\left( m \right)\)
- \(B_{0}\) :
-
Magnetic field strength
- \(T\) :
-
Nanofluid temperature \(\left( K \right)\)
- \(T_{w}\) :
-
Wall temperature \(\left( K \right)\)
- \(T_{\infty }\) :
-
Ambient temperature \(\left( K \right)\)
- \(C\) :
-
Nanoparticle volume fraction
- \(C_{\infty }\) :
-
Ambient nanoparticle volume fraction
- \(c_{p}\) :
-
Specific heat \(\left( {JK^{ - 1} kg^{ - 1} } \right)\)
- \(\rho c_{p}\) :
-
Heat capacity \(\left( {Jkg^{ - 3} K^{ - 1} } \right)\)
- \(q_{r}\) :
-
Radiative heat flux
- \(D_{B}\) :
-
Brownian diffusion coefficient \(\left( {m^{2} s^{ - 1} } \right)\)
- \(D_{T}\) :
-
Thermophoretic diffusion coefficient \(\left( {m^{2} s^{ - 1} } \right)\)
- \(u_{w}\) :
-
Velocity of the plate \(\left( {ms^{ - 1} } \right)\)
- \(Nu\) :
-
Local Nusselt number
- \(C_{f}\) :
-
Skin friction
- \(Sh\) :
-
Local Sherwood number
- \(Ec\) :
-
Eckert number
- \(Rd\) :
-
Radiation parameter
- \(Nt\) :
-
Thermophoresis parameter
- \(Nb\) :
-
Brownian motion parameter
- \(We\) :
-
Weissenberg number
- \(Pr\) :
-
Prandtl number
- \(M\) :
-
Magnetic parameter
- \(S_{0}^{\prime \prime \prime }\) :
-
Entropy generation rate \(\left( {JK^{ - 1} } \right)\)
- \(Be\) :
-
Bejan number
- \(\rho\) :
-
Density \(\left( {kgm^{ - 3} } \right)\)
- \(\sigma\) :
-
Electric conductivity \(\left( {kg^{ - 1} m^{ - 3} s^{3} A^{2} } \right)\)
- \(\theta\) :
-
Dimensionless temperature
- \(\phi\) :
-
Dimensionless concentration
- \({\Psi }\) :
-
Stream function
- \(\gamma\) :
-
Thermal relaxation constant
- \(\gamma_{1}\) :
-
Slip parameter
- \(\nu\) :
-
Kinematic viscosity \(\left( {Nsm^{ - 2} } \right)\)
- \(w\) :
-
Condition at the wall
- \(\infty\) :
-
Free stream condition
- \(^{\prime}\) :
-
Differentiation with respect to \(\eta\)
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Appendix
Appendix
To calculate the Eq. (24), we need
Now putting the above expression in Eq. (12), we get
Then further simplify we get
Now multiply the equation both sides by (1/a2x), thus
Using the thermophysical properties in Eq. (50), it becomes
Here, \(We = \sqrt {\frac{{2a^{3} }}{\upsilon }} \beta x,\,\,M^{2} = \frac{{\sigma B_{0}^{2} }}{a\rho },\,k_{p} = \frac{\upsilon }{{ak_{0} }},\)
Now to calculate the Eq. (25), we need
LHS term of Eq. (22), we have
Multiply with \(\frac{1}{a\Delta T}\)
Here \(\gamma = \lambda_{T} a\).
Right hand side term of Eq. (22), we have
Multiply with \(\frac{1}{a\Delta T}\)
Simply this we get
where \(\Pr = \frac{{\mu c_{p} }}{k},Rd = \frac{{4\sigma *T_{\infty }^{3} }}{kk*},Nb = \frac{{\tau D_{B} }}{\upsilon }C_{\infty } ,Nt = \frac{{\tau D_{T} }}{{T_{\infty } \upsilon }}\Delta T,Ec = \frac{{u_{w}^{2} }}{{c_{p} \Delta T}},\)
Finally, to calculate Eq. (26), we have
Multiply with \(\frac{1}{{aC_{\infty } }}\)
where \(Le = \frac{\alpha }{{D_{B} }}\).
Boundary conditions
at y = 0
where \(\gamma_{1} = \gamma *\sqrt {\frac{a}{\upsilon }} ,\,\,L_{1} = \xi *u_{w} \sqrt {\frac{a}{\upsilon }} .\)
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Gangadhar, K., Seshakumari, P.M., Venkata Subba Rao, M. et al. MHD Flow Analysis of a Williamson Nanofluid due to Thomson and Troian Slip Condition. Int. J. Appl. Comput. Math 8, 6 (2022). https://doi.org/10.1007/s40819-021-01204-1
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DOI: https://doi.org/10.1007/s40819-021-01204-1