Abstract
In nature, many fluid-like materials exhibit a yield stress below which they behave like a solid. The Bingham model aims to describe such materials. This paper draws some mathematical considerations on the flow of a Bingham fluid in a vertical channel. The situation due to the presence of an external magnetic field and natural convection is analyzed: the external magnetic field, which is orthogonal to the walls of the channel, generates the Lorentz forces that influence the motion through the Hartmann number. The behavior of the velocity, the induced magnetic field and the thickness of the plug regions are discussed and presented graphically. We find that the velocity is a decreasing function of the Bingham and Hartmann numbers. In particular, the presence of the external magnetic field increases the thickness of the plug region. The modulus of the induced magnetic field is not monotone when the Hartmann number changes, but it is a decreasing function of the Bingham number.
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Abbreviations
- b :
-
Thermal diffusivity (\(\hbox{m}^2 \,{\rm s}^{-1}\))
- B :
-
Bingham number (dimensionless parameter)
- C :
-
Constant such that \(P^*\) or \(p^* \,=\,-Cx_1 +p_0\) \({\text{(Nm}}^{{ - 3}} )\)
- \(\widetilde{C}_0\) :
-
Integration constant (\(\hbox{N}\, \hbox{m}^{-2}\))
- \(C_0\) :
-
Dimensionless integration constant
- \(\mathbf{D}\) :
-
Stretching tensor (\(\hbox{s}^{-1}\))
- 2d :
-
Distance between the walls (m)
- \({\mathbf{E}}\) :
-
Electric field (\(\hbox{V}\, \hbox{m}^{-1}\)), V = volt
- \((\mathbf{e}_1,\mathbf{e}_2,\mathbf{e}_3)\) :
-
Orthonormal basis of \({{\mathbb {R}}}^3\) (dimensionless)
- \(\mathbf{g}\) :
-
Gravity acceleration (\(\hbox{m}\, \hbox{s}^{-2}\))
- \(\mathbf{H}\) :
-
Total magnetic field (\(\hbox{A}\, \hbox{m}^{-1}\)),
- h(y):
-
Dimensionless function describing induced magnetic field
- \(H_0\mathbf{e_2}\) :
-
External uniform magnetic field (\(\hbox{A}\, \hbox{m}^{-1}\))
- \(H_1\mathbf{e_1}\) :
-
Induced magnetic field (\(\hbox{A}\, \hbox{m}^{-1}\))
- \(\mathbf{I}\) :
-
Identity tensor (dimensionless)
- k :
-
Thermal conductivity (\(\hbox{W}\, \hbox{m}^{-1} \hbox{K}^{-1}\))
- \(k_{1,2}\) :
-
Heat transfer coefficients at \(\Pi _{1,2}\) (\(\hbox{W}\, \hbox{m}^{-2} \hbox{K}^{-1}\))
- M :
-
Hartmann number (dimensionless parameter)
- \(Nu_{1,2}\) :
-
Nusselt numbers at the walls \(\Pi _{1,2}\) (dimensionless parameters)
- p :
-
Pressure (\(\hbox{N}\,\hbox{m}^{-2}\))
- \(p^*\) :
-
Modified pressure in the absence of an external magnetic field (\(\hbox{N}\,\hbox{m}^{-2}\))
- \(P^*\) :
-
Modified pressure in the presence of an external magnetic field (\(\hbox{N}\,\hbox{m}^{-2}\))
- \(p_0\) :
-
Some constant (\(\hbox{N}\,\hbox{m}^{-2}\)
- \({\mathbf{{q}}}\) :
-
Heat flux vector (\(\hbox{W}\, \hbox{m}^{-2}\))
- T :
-
Temperature (K)
- \(\mathbf{T}\) :
-
Stress tensor (\(\hbox{N}\, \hbox{m}^{-2}\))
- \({\mathbf{T}}^\text{D}\) :
-
Deviatoric part of \(\mathbf{T}\) (\(\hbox{N}\, \hbox{m}^{-2}\))
- \(T^\text{D}_\text{ij}\) :
-
Components of \({\mathbf{T}}^\text{D}\) (\(\hbox{N}\, \hbox{m}^{-2}\))
- \(t_{12}\) :
-
Dimensionless component of \({\mathbf{T}}^\text{D}\)
- \(T_0\) :
-
Reference temperature (K)
- \(T_{1,2}\) :
-
Uniform temperatures at the walls \(\Pi _{1,2}\) \((T_2 > T_1)\) (K)
- \(\mathbf{v}\) :
-
Velocity field (\(\hbox{m}\,\hbox{s}^{-1}\))
- v :
-
Dimensionless velocity
- \(V_0\) :
-
Characteristic velocity (\(\hbox{m}\,\hbox{s}^{-1}\))
- \(v_1\) :
-
Velocity component in \(x_1-\)direction (\(m\,s^{-1}\))
- \(x_1,\,x_2,\,x_3\) :
-
Cartesian coordinates (m)
- y :
-
Dimensionless transverse coordinate
- \(y_{0,1,2}\) :
-
Dimensionless boundaries of the plug regions.
- \(\alpha\) :
-
Thermal expansion coefficient (\(\hbox{K}^{-1}\))
- \(\eta _\text{e}\) :
-
Magnetic diffusivity \(\displaystyle \left( \eta _\text{e}=\frac{1}{\mu _\text{e}\sigma _\text{e}}\right)\) (\(\hbox{m}^2\,\hbox{s}^{-1}\))
- \(\vartheta\) :
-
Dimensionless temperature
- \({\mu}\) :
-
Dynamic viscosity coefficient (\(\hbox{N}\,\hbox{m}^{-2}\,\hbox{s}\))
- \({\mu _\text{e}}\) :
-
Magnetic permeability (\(\hbox{H}\, \hbox{m}^{-1}\))
- \(\rho _0\) :
-
Mass density at the temperature \(T_0\) (\(\hbox{Kg}\,\hbox{m}^{-3}\))
- \(\sigma _\text{e}\) :
-
Electrical conductivity (\(\hbox{S}\,\hbox{m}^{-1}\))
- \(\tau\) :
-
Yield stress (\(\hbox{N}\, \hbox{m}^{-2}\))
- \({\varvec{\tau }}_{1,2}\) :
-
Skin frictions at the walls \(\Pi _{1,2}\) (\(\hbox{N}\, \hbox{m}^{-2}\))
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Borrelli, A., Giantesio, G. & Patria, M.C. Exact solutions in MHD natural convection of a Bingham fluid: fully developed flow in a vertical channel. J Therm Anal Calorim 147, 5825–5838 (2022). https://doi.org/10.1007/s10973-021-10882-4
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DOI: https://doi.org/10.1007/s10973-021-10882-4