Abstract
The onset of convection in a porous medium saturated by the Oldroyd-type viscoelastic fluid, heated and salted from below, is investigated by incorporating the effects of chemical reactions on boundaries and externally imposed magnetic fields with non-equilibrium temperature conditions. The normal mode technique is used to perform linear stability analysis. The whole study is divided into two parts: (i) the parametric study for stability analysis in the oscillatory case and (ii) the stability analysis with the comparative study between different boundary conditions for controlling parameters for the limited case (in the stationary case, the viscoelastic effect is missing). These boundary surfaces are: (a) realistic bounding surfaces (i.e., rigid–free and free–rigid (R/R, R/F and F/R)) and (b) non-realistic bounding surface, i.e., free–free (F/F). For studying the viscoelastic fluid behavior, i.e., effect of the viscoelastic parameters (i.e., relaxation parameter \(({\lambda }_{1})\)) and retardation parameter \(({\lambda }_{2})\), we discussed the oscillatory state on free–free boundary surfaces. To analyze the consequences of different controlling parameters, numerical computation has been performed, and the results are illustrated in graphical form. For oscillatory convection, the minimum of the critical Rayleigh number drops as the relaxation parameter (\({\lambda }_{1})\), solute Rayleigh number (RaS) and Lewis number (Le) increase while it increases as the retardation parameter (\({\lambda }_{2})\), Chadrashekhar number (Q) and interphase heat transfer coefficient ( \(\tau )\) increase. In comparative study for stationary convection, the graphs demonstrate that while the critical Rayleigh number reduces as the value of Damk \(\ddot{o}\) hler number (\(\chi )\) grows, it increases along with increase in Chandrashekhar number (Q), interphase heat transfer coefficient (\(\tau )\) and Lewis number (Le).
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Abbreviations
- a :
-
Ve number [m−1]
- a c :
-
Critical wave number [m−1]
- d :
-
Height of the fluid layer [m]
- g :
-
Acceleration due to gravity [m/s2]
- \(\mathcal{H}\) :
-
Magnetic field
- K − 1 :
-
Inverse permeability
- Le:
-
Lewis number
- P :
-
Pressure [kg m−1 s−2]
- Pm:
-
Magnetic Prandtl number
- Q :
-
Chandrashekhar number
- Ra:
-
Rayleigh number
- RaS :
-
Solutal Rayleigh number
- \(\mathfrak{e}\) :
-
Solute concentration
- T f :
-
Temperature of fluid [kelvin]
- T s :
-
Temperature of solid [kelvin]
- t :
-
Time [s]
- U :
-
Velocity [ms−1]
- Va:
-
Vadasz number
- x, y, z :
-
Space coordinates
- β T :
-
Coefficient of thermal expansion
- β \(\mathfrak{e}\) :
-
Coefficient of solute expansion
- \(\varepsilon\) :
-
Porosity
- \({\eta }_{f}\) :
-
Fluid thermal conductivity ratio
- \({\eta }_{s}\) :
-
Solid thermal conductivity ratio
- \(\tau\) :
-
Dimensionless interphase heat transfer coefficient
- \({\lambda }_{1}\) :
-
Relaxation time
- \({\lambda }_{2}\) :
-
Retardation time
- χ:
-
Damk \(\ddot{o}\) hler number
- γ:
-
Ratio of heat capacities
- κf :
-
Thermal diffusivity
- κ\(\mathfrak{e}\) :
-
Solutal diffusivity
- \(\mu\) :
-
Dynamic viscosity of the fluid
- μ m :
-
Magnetic permeability
- σ :
-
Growth rate
- ρ :
-
Fluid density [kg m−3]
- Λ:
-
Magnetic viscosity
- \(\xi\) :
-
Anisotropy ratio
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Author Monal Bharty greatly acknowledges the financial assistance from Central University of Jharkhand as a research fellowship.
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Bharty, M., Srivastava, A.K. & Mahato, H. The effect of chemical reaction on thermo-solutal magneto-convection under non-equilibrium temperature conditions. Int J Adv Eng Sci Appl Math (2024). https://doi.org/10.1007/s12572-024-00368-5
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DOI: https://doi.org/10.1007/s12572-024-00368-5