Casson Fluid Flow Due to Non-Coaxial Rotation of a Porous Disk and the Fluid at Infinity Through a Porous Medium

Rafiq, Shahid; Nawaz, M.; Mustahsan, Muhammad

doi:10.1134/s0021894418040053

Cited by 7 publications

(5 citation statements)

References 12 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The heat transfer is due to the dissipation and thermal radiation; and the solution to the problem was obtained using HAM. Rafiq et al 26 considered the flow of Casson fluid between two porous co-axial rotating disks; the flow was assumed to be unsteady with disks being in two and fro motion and both upper and lower disk are subject to suction/injection effect. Hayat et al 27 examined the flow characteristics of Casson fluid flowing between rotating disks; the flow was assumed to be mixed convective and the system was exposed to physical process like chemical reaction, thermal radiation, convective heating and uniform source/sink of heat.…”

Section: Introductionmentioning

confidence: 99%

Particle Swarm Optimization for exploring Darcy–Forchheimer flow of Casson fluid between co-axial rotating disks with the Cattaneo–Christov model

Uddin,

Upreti,

Ganga

et al. 2024

Sci Rep

View full text Add to dashboard Cite

In this paper, we carried out a numerical analysis of the fluid dynamics and heat transfer occurring between two parallel disks. The study accounts for the impact of temperature-dependent fluid viscosity and thermal conductivity. We systematically investigated various parameters, including viscosity, thermal conductivity, rotational behavior (rotation or counter-rotation), and the presence of stretching, aiming to comprehend their effects on fluid velocity, temperature profiles, and pressure distributions. Our research constructs a mathematical model that intricately couples fluid heat transfer and pressure distribution within the rotating system. To solve this model, we employed the 'Particle Swarm Optimization' method in tandem with the finite difference approach. The results are presented through visual representations of fluid flow profiles, temperature, and pressure distributions along the rotational axis. The findings revealed that the change in Casson factor from 2.5 to 1.5 resulted in a reduction of skin friction by up to 65%, while the change in local Nusselt number was minimal. Furthermore, both the viscosity variation parameter and thermal conductivity parameters were found to play significant roles in regulating both skin friction and local Nusselt number. These findings will have practical relevance to scientists and engineers working in fields related to heat management, such as those involved in rotating gas turbines, computer storage devices, medical equipment, space vehicles, and various other applications.

show abstract

Section: Introductionmentioning

confidence: 99%

Particle Swarm Optimization for exploring Darcy–Forchheimer flow of Casson fluid between co-axial rotating disks with the Cattaneo–Christov model

Uddin,

Upreti,

Ganga

et al. 2024

Sci Rep

View full text Add to dashboard Cite

show abstract

“…Loganathan and Deepa 34 investigated the flow of convective Casson fluid paste a Riga plate. Rafiq 35 studied Casson fluid flow generated by the non-coaxial rotation of a disk. Exact solutions of BVP are obtained by using Laplace transform technique.…”

Section: Introductionmentioning

confidence: 99%

Time fractional analysis of channel flow of couple stress Casson fluid using Fick’s and Fourier’s Laws

Ahmad

Haq

Ali

et al. 2022

Sci Rep

View full text Add to dashboard Cite

This study aim to examine the channel flow of a couple stress Casson fluid. The flow is generated due to the motion of the plate at $$y=0$$ y = 0 , while the plate at $$y=d$$ y = d is at rest. This physical phenomenon is derived in terms of partial differential equations. The subjected governing PDE’s are non-dimensionalized with the help of dimensionless variables. The dimensionless classical model is generalized by transforming it to the time fractional model using Fick’s and Fourier’s Laws. The general fractional model is solved by applying the Laplace and Fourier integral transformation. Furthermore, the parametric influence of various physical parameters like Casson parameter, couple stress parameter, Grashof number, Schmidt number and Prandtl number on velocity, temperature, and concentration distributions is shown graphically and discussed. The heat transfer rate, skin friction, and Sherwood number are calculated and presented in tabular form. It is worth noting that the increasing values of the couple stress parameter $$\lambda$$ λ deaccelerate the velocity of Couple stress Casson fluid.

show abstract

“…Ersoy [43] imposed a disk with non-torsional oscillation to study the convective non-coaxial rotating flow for a Newtonian fluid. Mohamad et al [44,45] worked on similar study considering the second grade fluid and Rafiq et al [46] concerning the Casson fluid model. The time dependent flow of an incompressible fluid with MHD, chemical reaction and radiation effects under non-coaxial rotation was investigated by Rana et al [47].…”

Section: Introductionmentioning

confidence: 99%

Analysis of Heat Transfer in Non-Coaxial Rotation of Newtonian Carbon Nanofluid Flow with Magnetohydrodynamics and Porosity Effects

Noranuar¹,

Mohamad²,

Shafie³

et al. 2022

21st Century Nanostructured Materials - Physics, Chemistry, Classification, and Emerging Applications in Industry, Biomedicine,

View full text Add to dashboard Cite

The study analyzed the heat transfer of water-based carbon nanotubes in non-coaxial rotation flow affected by magnetohydrodynamics and porosity. Two types of CNTs have been considered; single-walled carbon nanotubes (SWCNTs) and multi-walled carbon nanotubes (MWCNTs). Partial differential equations are used to model the problem subjected to the initial and moving boundary conditions. Employing dimensionless variables transformed the system of equations into ordinary differential equations form. The resulting dimensionless equations are analytically solved for the closed form of temperature and velocity distributions. The obtained solutions are expressed in terms of a complementary function error. The impacts of the embedded parameters are graphically plotted in different graphs and are discussed in detail. The Nusselt number and skin friction are also evaluated. The temperature and velocity profiles have been determined to meet the initial and boundary conditions. An augment in the CNTs’ volume fraction increases both temperature and velocity of the nanofluid as well as enhances the rate of heat transport. SWCNTs provides high values of Nusselt number compared to MWCNTs. For verification, a comparison between the present solutions and a past study is conducted and achieved excellent agreement.

show abstract

Casson Fluid Flow Due to Non-Coaxial Rotation of a Porous Disk and the Fluid at Infinity Through a Porous Medium

Cited by 7 publications

References 12 publications

Particle Swarm Optimization for exploring Darcy–Forchheimer flow of Casson fluid between co-axial rotating disks with the Cattaneo–Christov model

Particle Swarm Optimization for exploring Darcy–Forchheimer flow of Casson fluid between co-axial rotating disks with the Cattaneo–Christov model

Time fractional analysis of channel flow of couple stress Casson fluid using Fick’s and Fourier’s Laws

Analysis of Heat Transfer in Non-Coaxial Rotation of Newtonian Carbon Nanofluid Flow with Magnetohydrodynamics and Porosity Effects

Contact Info

Product

Resources

About