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Research Article
2025
:37;
9662025
doi:
10.25259/JKSUS_966_2025

Reiner-rivlin nanofluid behavior with gyrotactic microorganisms and slip conditions in a rotating disk configuration

Department of Mathematics, College of Science and Humanities in Al-Kharj, Prince Sattam bin Abdul-AzizUniversity, Al-Kharj, 11942, Saudi Arabia
Department of Basic Engineering Science, Faculty of Engineering, Menofia University, ShebinEl-Kom 32511, Egypt
Department of Mathematics and Sciences, Sir Syed University of Engineering and Technology, Karachi, Pakistan
School of Science, Walailak University, Nakhon Si Thammarat 80160, Thailand
Research Center for Theoretical Simulation and Applied Research in Bioscience and Sensing, Walailak University, Nakhon Si Thammarat 80160, Thailand
Department of Electrical Engineering, College of Engineering, Princess Nourah bint Abdulrahman University, P.O. Box 84428, Riyadh 11671, Saudi Arabia
Center for Scientific Research and Entrepreneurship, Northern Border University, 73213, Arar, Saudi Arabia
Department of Mathematical Sciences, Federal Urdu University of Arts, Sciences & Technology, Gulshan-e-Iqbal Karachi, 75300
Sciences and Mathematics Unit, Department of Supportive Requirements, University of Technology and Applied Sciences, Salalah, Sultanate of Oman. P.O.Box 608, PC:211, Salalah, Sultanate of Oman

Corresponding author E-mail address: anwartalha80@gmail.com (T. Anwar)

Licence
This is an open-access article distributed under the terms of the Creative Commons Attribution-Non Commercial-Share Alike 4.0 License, which allows others to remix, transform, and build upon the work non-commercially, as long as the author is credited and the new creations are licensed under the identical terms.

Abstract

In the realm of fluid mechanics, the behavior of materials often defies simplistic characterization, requiring sophisticated models to capture their intricate dynamics, especially when involving non-Newtonian fluids. This research endeavors to elucidate the bioconvection flow of Reiner-Rivlin nanofluid incorporating gyrotactic microorganisms in the presence of magnetohydrodynamics (MHD), multiple slip, and thermal radiation over a rotating surface. Thermal and solutal convective boundary conditions have also been considered. The Buongiorno model is added together with the governing equations in partial differential equations (PDEs). By the adoption of transformation, the complex PDEs are transformed into ordinary differential equations (ODEs). The physical quantities of interest in this study are drag friction, heat, mass, and local motile microorganism density. Numerical solutions are calculated by the bvp4c solver in MATLAB, and the impacts of the governing parameters are visualized through graphical representations and tabulated data. Visual representations are used to inspect the significant effects of the changing parameters on the involved fields. The results demonstrate that radial velocity and temperature are improved for a strong Reiner-Rivlin material parameter. Enhancing slip variables lessens the shear stress by up to 30%, considerably. Tables show the relation between various estimations of emergent parameters and the behavior of microorganism density, friction coefficients, rate of heat and mass are provided. By comparing the reported results to an existing published study, we can verify that the intended model is authentic. We get a proper correlation between the two sets of results. These findings emphasize the possibility for enhancing refrigeration procedures for spinning systems like windmills and disk-based thermal exchangers by combining viscous nanofluids and microbial growth. This study sheds light on the development of innovative bio-nanofluidic technologies and effective heat control techniques for commercial and medical uses.

Keywords

Entropy generation
MHD flow
Nanofluid
Reiner-rivlin flow
Thermal radiation

1. Introduction

Fluid mechanics is a scientific study focused on how external forces affect the structure within fluids. It represents a division of classical physics through significant features in zoology, aerospace engineering, chemical engineering, and mechanical engineering. Two sorts of fluids are non-Newtonian and Newtonian fluids. Newtonian fluids adhere to linear relationships between stress and strain, meaning the fluid’s resistance to deformation is constant; meanwhile, non-Newtonian fluids exhibit more complex behaviors, often requiring sophisticated models for accurate description. The Reiner-Rivlin fluid was one of the non-Newtonian fluids, which (Reiner 1945) and (Rivlin 1948) described as unique characteristic of dilatancy. This characteristic refers to the viscoelastic tendency to expand in volume when agitated. (Selvi and Shukla 2022) presented a theoretical investigation to notice an analytical procedure of a micropolar fluid through a sphere by adopting the Mehta-Morse boundary condition. Their work separated the flow into two parts: the outer region fills with the micropolar fluid, while the Reiner-Rivlin fluid regulates the inner flow. They found that the drag is less resistant to a Reiner-Rivlin liquid sphere than to an impermeable sphere. The study on the rate of energy and concentration flux through a revolving stretch disc using the Cattaneo-Christov model adopting the Stefan blowing was published by (Moatimid et al., 2022). The model equations were solved through Homotopy perturbation (HPM). They observed that the rate of heat and mass transport is enhanced through Stefan-blowing particle diffusion. Some medical therapies were able to benefit from this finding. (Puspa Nathan et al., 2024) indicated the impact of Reiner-Rivlin due to the shrinking/stretching rotating disk. They noticed that a dual solution occurs in some range of parameters when the effects are added to the flow. A few series of literature based on the Reiner-Rivlin fluid with several effects over different surfaces can be seen in (Arain et al., 2021; Hiremath et al., 2023; Hayat T et al., 2023; Alarabi et al., 2023; Yasin et al., 2025).

The concept of rotating flow was pioneered by Kármán et al. (1921) by postulating an infinitely large disk spinning at a constant angular velocity within a quiescent fluid medium. Centrifugal compressors and fans are based on this design, which uses a rotating disk to push fluid. However, the centrifugal forces are sufficiently weak to cause the fluid to depart radially due to the disk’s surface. Consequently, the displaced fluid is replenished by the fluid layer located overhead the disk, facilitated by a disk pumping result characterized by descending spiralling motion. The replication of the flow of fluid due to a revolving disk was first described by Cochran (1934). Since then, the work on the flow over rotating disks has sparked curiosity among researchers, especially in the application of power turbines, circulating lubrication, the geothermal industry, and so on. Followed by Smith (1947), who was the first to investigate the boundary layer transition using hot-wire techniques. In his study, he observed that the sinusoidal disturbances appear in the disk boundary layer at sufficiently large Reynolds numbers. Meanwhile, (Imayama et al., 2016) constructed an experimental study with surface roughness. (Thomas et al., 2023) studied the role of wall slip across the linear stability of the spinning disc. The heat transport of inclined flow of the rotating disc under magnetohydrodynamics (MHD) was inspected by Mahmud et al. (2023) using the shooting method. They observed that the strengthening magnetic field and the increase in the rotating disc enhance the heat transfer of the flow. (Faizan et al., 2024) considered the stagnant flow of the Maxwell nanomaterial across a stretching/shrinking spinning disk and solved it using bvp4c in MATLAB.

The term and phenomenon of bioconvection were used by Loefer et al. (1952) and Platt (1961). According to Pedley et al. (1988), bioconvection is the phenomenon where the fluids exhibit macroscopic motion driven by density gradients generated by the coordinated movement of motile microorganisms. Additionally, research on microorganisms has garnered significant attention from researchers due to their widespread applications in commercial, industrial, and microbiological systems. These applications span a variety of fields, including biofertilizers, bioinformatics, alcohol production, biotechnology, biofuel generation, and biosensors. For instance, microalgae represent a rapidly growing biomass that can be utilized in the production of bio-based materials, alcohol, and biofuels. (Kuznetsov 2010) deliberates the problem of convection with nanofluid considering gyrotactic microorganisms. The main aim of microorganisms is to enhance or induce nanofluid convection. Later, Kuznetsov (2021) continued the study of the nanofluid alongside motile (oxytactic) microorganisms to understand the behavior while inspecting its stability when it occupies a shallow horizontal layer. (Othman et al., 2023) solved the problem comprising the gyrotactic microbe through a stretchable inclined cylinder with heat and mass transfer characteristics. In their study, the thermal layer was enhanced with larger values of heat source sink while reduced with larger magnitudes of Prandtl number. Nabwey et al. (2022) investigated the problem of bioconvection involving gyrotactic microorganisms in a porous surface. In their problem, the problem is numerically solved using the Runge-Kutta procedure and shooting technique. Li et al. (2023) scrutinized the environmental transport of gyrotactic microorganisms in an open-channel flow. Flow shear’s impact remains negligible on the overall shape of the asymptotic concentration distribution. Nevertheless, it has a pronounced effect in significantly augmenting both the transient drift velocity and dispersity. Few studies based on bioconvective gyrotactic microorganisms can be seen from these aforementioned works (Dawar et al., 2021; Algehyne et al., 2023; Fatima et al., 2023; Sarma et al., 2024; Abbas et al., 2024).

The influence of boundary slip in fluids holds significant implications, particularly in features that involve refining artificial cardiac chambers and inside cavities. Speed and energy play crucial roles in governing the fluid flow at the micro-scale. Wall slip behavior plays a great role due to its examination for drag reduction in aerodynamics and hydrodynamics. Navier made his debut with the Navier-Stokes algorithm, which is a popular tool for enhancing fluid flows. (Ramya et al., 2018) discovered the MHD past a non-linear stretchable surface through momentum and thermal slip. They found that the rate of heat and mass transport decreases with the growing magnitude of thermal slip. Yang et al. (2020) explored the effect of viscoelastic second-order slip for the flow of Maxwell fractional fluid. The finite difference method was employed to solve the governing fluid model. The findings indicate that the fractional Maxwell fluid demonstrates enhanced viscosity or elasticity across various fractional parameters. The impact of Navier’s slip and MHD over a porous surface for non-Newtonian fluid is investigated by Maranna et al. (2023). In their work, they chose Ag-Cu, which is presented in the blood as a viscous fluid. It is found that the rising concentration of Ag-Cu intensification the thermal layer. Sharma et al. (2023) studied MHD micropolar fluid through a stretching surface with melting and slip effects. The impact on buoyancy and heat sources over a separation of the unsteady stagnation point was explored by Mahmood et al. (2024). The unsteadiness parameter for opposing flow improved skin friction.

By addressing the limitation, this paper aims to explore von Kármán flow and heat transfer phenomena within a MHD flow of Reiner-Rivlin non-Newtonian fluid over a rotating surface, considering thermal radiation effects and multiple slip conditions with heated and concentration boundary conditions. The previous study was explained by Khan et al. (2024). We have extended their work, added multiple slip effects, and thermal/solutal convective conditions past a rotating disk. Incorporating multiple slip effects offers advantages, particularly in engineering applications, enabling more accurate predictions of flow behavior as well as in the optimization process. Additionally, the inclusion of thermal radiation in the analysis of Reiner-Rivlin fluids will provide a comprehensive understanding of heat transfer performance and fluid behavior. These findings have the potential to enhance simulation accuracy and facilitate the optimization of industrial processes.

2. Physical Problem and Model Formulation

The steady, 3D flow of Reiner-Rivlin Nano liquid containing gyrotactic bacteria that move on a disk that is turning. Nanofluid rotates around the zaxis, which is parallel to the surface, at an angle Ω, with u, v, and w being the speeds along r, ϕ, and z has been deliberated in Fig. 1(a). It is considered that Tf,Cf and χw , and T , C , χ are the fluid temperature, concentration, and the number of moving microbes near and far from the surface. The flow problem’s highly nonlinear solutions are changed into normal ones that are similar enough. This is what we did with the bvp4c plan. We can find the tensor of the Reiner-Rivlin fluid by Reiner (1945) and Rivlin (1948).

(a) Physical geometry of the rotating flow, (b) Numerical method Bvp4c flow chart.
Fig. 1.
(a) Physical geometry of the rotating flow, (b) Numerical method Bvp4c flow chart.

The stress tensor of the Reiner-Rivlin model is described as:

1
τij =pδij +μeij +μc eik ekj ;ejj

Here, eij = ui xj + uj xi , p,μ, δij , ejj , μc is pressure, dynamic viscosity of coefficient, Kronecker delta, deformation rate tensor, and cross-viscosity coefficient.

The constitutive equations are explained as

2
u r +ur+ w z =0

3
ρ u u r v2 r+w w z = τrr r + τrz z + τrr τϕϕ r + 1 ρf 1 Cf ρf β1 g TT ρpρf g C C β2 ρmρf g χχ σB0 2 uρ        

4
ρzxa u u r + uvr+w v z = 1 r2 r r2 τrϕ + τrϕ z + τrϕ τϕr r σB0 2 vρ

5
ρ u w r +w w z = 1r r r τrz + τzz z

The stress tensor for the deformation is (Rivlin 1948)

6
err =2 u r ,eϕϕ =2 ur,ezz =2 w z ,erϕ =eϕr =rr vr , ezϕ =eϕz = v r ,ezr =ezr = u z + w r

Stress tensor components are considered as (Selvi and Shukla, 2022, and Sabu et al., 2016):

7
τrr =p+μ2 u r +μc 4 u r 2 + u r + w r 2 + v r vr 2

8
τzr =μ u z + w r +μc u z + w r 2 2 u r + v z v r v r + 2 w z u z + w r

9
τϕϕ =p+μ 2 ur +μc 4 ur 2 + v z 2 + v r vr 2

10
τzr =μ u z + w r +μc u z + w r 2 2 u r + v z v r v r + 2 w z u z w r

11
τrϕ =μ v r vr +μc v r vr 2 2 u r + 2ur v r vr + v z u z + w r

12
τzϕ =μ v z +μc u z + w r 2 v r vr +2 v z ur + w z v z

13
τzz =p+2μ w z +μc 4 w z 2 + v z 2 + u z + w r 2

Using Eqns. (3) – (5)

14
u u r v2 r+w u z =ν 2 u z2 + μc ρ 4 u z 2 u rz +2 u r 2 u z2 +2 w z 2 u z2 + 2 v z2 v z vr + v z 2 v zr 1r v z +2 u z 2 w z2 + 1r u z 2 v z 2 1 ρf 1Cf ρf β1 g TT ρpρf g CC β2 ρmρf g χχ σB0 2 uρ

15
u v r + uvr+w v z =ν 2 v z2 + μc ρ v z 2 u zr + u z 2 v zr + 4r u z v z 2 u z2 v z vr + u z 2 v zr 1r v z +2 w z 2 v z2 +2 v z 2 w z2 σB0 2 vρ

16
u T r +w T z = αf+ 16 σ* T3 3k  (ρCp)f 2 T r2 + 1r T r + 2 T z2 +τ DB C z T z + DT T T z 2 + Q0 (ρCp)f TT

17
u C r +w C z =DB 2 C z2 + DT T 2 T z2 Kr2 T T nexp E0 κT (C C)

18
u χ r +w χ z = bWc χwχ z χ C z +DN 2 χ z2

Boundary conditions for the above problem are (Imamaya et al., 2016)

19
u=δ1 τzr , v=δ2 τzϕ +rΩ, w=0,k1 T z =h TfT ,k2 T z =h CfC , χ=χw at z=0. u0, v0,w0,TT, CC,χχ at z

Here, T, C, χ represent the temperature, concentration, and motile density of the fluid, respectively. Then, (ρc)p is nanoparticle tendency, αm is thermal diffusivity, (ρc)f is base fluid tendency, C is ambient concentration, k denotes thermal conductivity, χw is motile microorganism, Tf is temperature of the fluid, Cf is concentration of the surface. T is ambient temperature, χ is motile microorganism, DB is Brownian diffusivity, and DT is thermal diffusivity,

The suitable transformation is given below (Arain et al., 2021)

20
ξ= Ωυz , u=rΩF',v=rΩG,w=2 Ωυ F,μΩ,Pξ=PP ϑξ= TT TfT ,Φξ= CC CfC ,ϒξ= χχ χwχ

Utilizing Eq. (20), Eqns. (14) - (18) reduces to

21
F'''+ϵ(F''2 G'2 2F'F''')F'2 +G2 +2FF''+γ(ϑNrΦNcϒ)MF'=0

22
G''2F'G+2FG'+2λ(F''G'F'G'')MG=0

23
(1+4 / 3Rd)ϑ''+2PrFϑ'+Pr(Nbϑ'Φ'+Ntϑ'2 +Qϑ)=0

24
Φ+2ScFΦ+ Nt Nb ϑScCr (1+Λϑ)nexp Αe 1+Λϑ Φ=0

25
ϒ''+2LbFϒ'Pe Φ'' ϒ+ω +ϒ'Φ' =0

The converted boundary conditions are

26
F(0)=0,F(0)=β1 F(0)[12F(0)]+1, G(0)=β2 G'(0)[12F'(0)]+1, ϑ'(0)=Bit(1ϑ(0)),Φ'(0)=Bic(1Φ(0))=0,Υ(0)=1,atξ=0. F'0,G0,ϑ0,Φ0,ϒ0 asξ

Where, β1 shows radial slip, β2 azimuthal slip, M is a magnetic number, λ is Reiner-Rivlin fluid parameter, Nr is the buoyancy ratio variable, Nc is the bio covection Rayleigh number, Nb is Brownian motion Rd represents thermal radiation, Bit exhibits the thermal Biot number,Bic exhibits the solutal Biot number, Αe is the activation energy, Cr is a chemical reaction, Pr is Prandtl number, Sc exhibits Schmidt number,Nt is a thermophoretic parameter ω microorganism difference parameter, Lb is bio connection Lewis number, Pe is the Peclet number.

λ= μcΩμ , β1 = ρ Ωv δ1 , β2 = ρ Ωv δ2 ,M= σB0 2 ρ , Nr= ρpρf CfC β 1Cf TfT ρf Nc= ρmρf χfχ β 1Cf TfT ρf ,Rd= 16σ* T3 3k* k0 ,Bit= hf k1 vf Ω ,  Bic= hf k2 vf Ω , Ae= E0 kT ,Nb= τDB CfC v ,Nt= τDT TfT T˜v , Pr= μcp k ,Sc= v DB ,ω= χ χwχ ,Lb= v DN ,Pe= bWcv

3. Quantity of Engineering Importance

The least moment of torque is represented by Cm,r (Selvi and Shukla 2022):

27
Cm,r = Tr ρΩ2 r5

Tr signifies with uniform disk rotation

28
Tr= 0r τzϕ |z=0 2πr2 dr=π2 ρΩ vΩ r4 G' 0 .

The physical quantities of Cf,Nu,Sh and Nh is given as:

29
Cf= τr2 τϕ2 ρ (rΩ) 2 ,Nu= rqw k(TfT) , Sh= rjw DB(CfC) ,Nh= rjn DN(χwχ) ,

Using Eq. (19), Eq. (28) becomes

30
Cf Ωr2 v 1/2 = (F'' 0 ) 2 G''(0 )2 , Nu Ωr2 v 1/2 =(1+4/3Rd)ϑ' 0 , Sh Ωr2 v 1/2 =Φ 0 ,Nh Ωr2 v 1 2 =ϒ' 0 ,

4. Numerical Solution Methodology

The Bvp4c has been used for solving the configuration of nonlinear equations (21) - (25) with particular boundary condition (26) by MATLAB software. The nonlinear equations are converted into first order equations by assigning the new variables.

http://www.w3.org/1998/Math/MathML
F=Β1 ,F=Β2 ,F=Β3 ,G=Β4 ,G=Β5 ϑ=Β6 ,ϑ'=B7 ,Φ=B8 ,Φ'=B9 ,ϒ=B 10 ,ϒ'=Β 11 F'''+λ(F''2 G'2 2F'F''')F'2 +G2 +2FF''+γ(ϑNrΦNcϒ)MF'

31
B 3 = λB5 2 λB3 2 + B2 2 B4 2 λ2 B1 B3 +MB1 γ Β6 NrΒ8 NcΒ 10 12λB2

32
B5'= 2 B2 B4 2λB3 B5 2 B1 B5 +MB4 12λB2

33
B7'= 2PrB1 B7 Pr NbB7 B9 +NtB6 2 1+4/3Rd

34
B9'= ScCr (1+ΛP6 )nexp Ae 1+ΛP6 P8 2ScP1 P8 Nt Nb P7'

35
B 11 '=2LbB1 B 11 Pe B9' B 10 +ω +B 11 B9

Subsequently, boundary conditions are

36
B1 =0,B2 =β1 B3 12λB2 ,B4 =β2 B5 12λB2 +1, B7 =Bit 1B6 ,B9 =Bic 1B8 ,B 10 =1 B2 0,B4 0,B6 0,B8 0,B 10 0.

It is important to carefully choose the starting assumptions in these numerical simulations to make sure that the solution will meet the initial conditions. Many times, of the iterations have been done to get to a convergent result. Compared to other ways of doing analysis, these answers are very good. In most cases, the above-mentioned convergence criteria are used as a help to decide what values should be assigned to the given parameters. Each iteration of the process is run with a new parameter number as its starting point.

the use of a finite value for ξmax using the condition in Eqn. (36) is calculated by

37
F' (ξ) max ,G (ξ) max ,ϑ (ξ) max ,Φ (ξ) max ,ϒ (ξ) max

To get a numerical solution, convergent criteria are preferred, and the step size is set at Δξ = 0.0001 . The numerical flow chart has been described in Fig. 1(b).

5. Numerical validation of the BVP4c code

A comparison of the skin friction coefficient F''(0) and G(0) are compared with wall slip parameters β1 and β2 values are compared to those published in previous studies to assess the validity of the present numerical code. Tables 1 and 2 exhibit this by comparing the validity of the current research to previous investigations by (Abdal et al., 2021). The data confirms that the present results validate and reinforce the findings of previous studies, indicating strong agreement and reliability in the observed trends.

Table 1. Comparison of F''(0) current results with previous results.
β1 β2 (Abdal et al., 2021) Our results
0.0 0.0 0.5102326 0.51021
1.0 1.0 0.1279236 0.12792
5.0 5.0 0.0185885 0.01853
10.0 10.0 0.0068125 0.00684
20.0 20.0 0.0023614 0.00021
40.0 40.0 0.0007899 0.00073
Table 2. Comparison of G'(0) current results with previous results.
β1 β2 (Abdal et al., 2021) Our results
0.0 0.0 0.6159220 0.61597
1.0 1.0 0.3949275 0.39497
5.0 5.0 0.1433882 0.14335
10.0 10.0 0.0810300 0.08106
20.0 20.0 0.0437883 0.04378
40.0 40.0 0.0229952 0.02292

6. Results and Discussion

An incompressible mixed convection flow of Reiner-Rivlin nanoparticles with multiple effects across a rotating extended warmed disk is investigated in the presence of microorganisms. Nondimensional ordinary differential equations (ODEs) (20) – (24) with boundary conditions equation (25) are analyzed using the Bvp4c technique. The results are presented to show how various limits impact the problem, which helps to physically explain it. Among these factors are the following: the volume fraction slip parameter β1 ,β2 , magnetic field M, Reiner-Rivlin fluid factor ϵ, mixed convective parameter γ, buoyancy ratio parameter Nr, bioconvection Rayleigh number Nc, biot number Bit, the Brownian movement limit Nb, solutal biot number Bi, the thermophoresis limitation Nt, the, the Schmidt numeral Sc, activation energy Ae, Peclet number Pe. The effects of these restrictions on the velocities, temperatures, nanoparticle profiles, skin friction Cf, Nusselt Nu, and Sherwood Sh variables are the primary focus of the current investigation. The data described are used to plot these distributions are seen in Figs. 2-9. For the entire study, we kept the variables β1 =0.3, β2 =0.3,M=0.4,ε=0.1,γ=0.2,Nr=0.2,Nc=0.2,Nb=0.2,  Nt=0.1,Bit=0.2,Bic=0.2,Sc=1.0,Pe=1.0,Lb=1.0, Ae=1.0.

(a) Variation of M against Axial velocity Fξ , (b) Variation of M against Radial velocity F'ξ , (c) Variation of M against tangential velocity Gξ .
Fig. 2.
(a) Variation of M against Axial velocity Fξ , (b) Variation of M against Radial velocity F'ξ , (c) Variation of M against tangential velocity Gξ .
(a) Variation of ϵ against Axial velocity Fξ , (b). Variation of ϵ against Radial velocity F'ξ , (c) Variation of ϵ against tangential velocity Gξ .
Fig. 3.
(a) Variation of ϵ against Axial velocity Fξ , (b). Variation of ϵ against Radial velocity F'ξ , (c) Variation of ϵ against tangential velocity Gξ .
(a) Variation of γ against Radial velocity F'ξ , (b). Variation of β1 ,β2  against Radial velocity F'ξ .
Fig. 4.
(a) Variation of γ against Radial velocity F'ξ , (b). Variation of β1 ,β2  against Radial velocity F'ξ .
(a). Variation of ϵ against temperature profile ϑξ , (b). Variation of M against temperature profile ϑξ , (c). Variation of Nb against temperature profile ϑξ , (d). Variation of Nt against temperature profile ϑξ , (e). Variation of Pr against temperature profile ϑξ , (f). Variation of Rd against temperature profile ϑ(ξ)
Fig. 5.
(a). Variation of ϵ against temperature profile ϑξ , (b). Variation of M against temperature profile ϑξ , (c). Variation of Nb against temperature profile ϑξ , (d). Variation of Nt against temperature profile ϑξ , (e). Variation of Pr against temperature profile ϑξ , (f). Variation of Rd against temperature profile ϑ(ξ)
(a) variation of Nb against concentration profile Φξ , (b) variation of Nt against concentration profile Φξ , (c) Variation of Sc against concentration profile Φξ , (d) variation of Cr against concentration profile Φξ
Fig. 6.
(a) variation of Nb against concentration profile Φξ , (b) variation of Nt against concentration profile Φξ , (c) Variation of Sc against concentration profile Φξ , (d) variation of Cr against concentration profile Φξ
(a). Variation of Pe against microorganism density profile Υξ , (b). variation of Lb against microorganism density profile Υξ .
Fig. 7.
(a). Variation of Pe against microorganism density profile Υξ , (b). variation of Lb against microorganism density profile Υξ .
(a). Variation of M,λ against Cf, (b) variation of Rd, Pr against Nu, (c) variation of Ae,Sc against Sh, (d) variation of Pe,Lb against Nh
Fig. 8.
(a). Variation of M,λ against Cf, (b) variation of Rd, Pr against Nu, (c) variation of Ae,Sc against Sh, (d) variation of Pe,Lb against Nh
(a). Plot for grid analysis for Fξ , (b). Plot for grid analysis for F'ξ , (c). Plot for grid analysis for Gξ , (d). Plot for grid analysis for ϑξ , (e). Plot for grid analysis for Φξ , (f). Plot for grid analysis for Υ(ξ).
Fig. 9.
(a). Plot for grid analysis for Fξ , (b). Plot for grid analysis for F'ξ , (c). Plot for grid analysis for Gξ , (d). Plot for grid analysis for ϑξ , (e). Plot for grid analysis for Φξ , (f). Plot for grid analysis for Υ(ξ).

6.1 Fluid velocity

Figs. 2(a-c) display the magnetic variable M for possible values of wall slip variable ( β1 =β2 =0, β1 =β2 =0.3 ) affects the axial velocity Fξ , radial velocity F ξ , azimuthal velocity Gξ . Fig. 2(a) views the influence on the axial velocity Fξ with variation of magnetic variable M. Larger estimation of the magnetic field reduces the axial velocity Fξ . A higher magnetic variable M number means that there is more resistance (Lorentz forces), which slows down the flow in all three velocities. From Figs. 2(b-c), the similar trend is noted for the radial velocity F ξ , azimuthal velocity Gξ for the scenario of ( β1 =β2 =0,β1 =β2 =0.3 ). Figs. 3(a-c) appearance the Reiner-Rivlin fluid parameter ϵ curves when the variable ( β1 =β2 =0,β1 =β2 =0.3 ) for the axial velocity Fξ , radial velocity F ξ , azimuthal velocity Gξ . Figs. 3(a-b) displays the mechanism of Reiner-Rivlin fluid parameters upon the axial velocity Fξ and radial velocity F ξ . Escalating Reiner-Rivlin fluid parameters go up near the disk, axial velocity Fξ , radial velocity F ξ go down, while they go up farther away. As the vertical distance goes down, the absolute maximum also happens when K goes up. When viscoelastic effects are increased, more fluid is moved in the radial direction and less fluid is pulled in the axial direction. From what was said above, we can see that the traditional von Kármán problem keeps the centrifugal fan-like behavior in the non-Newtonian case. From the Fig. 3(c), the azimuthal velocity profile Gξ changes as the Reiner-Rivlin fluid parameter value ϵ increases. The effect of convective variable γ on F'ξ has been shown in Fig. 4(a). As the convective variable γ increases, the radius of the rotating disk enhances, which means that more fluid is in contact with the rotating, which surges up the flow. The behaviour of the wall slips parameters β1 ,β2 on F'ξ has been exposed in Fig. 4(b). When wall slip parameters β1 ,β2 went up, fluid viscosity enhanced, which made F'ξ go up.

6.2 Fluid temperature

Now, at the same time, the fluid gives off its movement energy as heat, taking the temperature up, which has been seen in Fig. 5(a). The role of Reiner-Rivlin fluid parameters ϵ for the thermal curve has been revealed in Fig. 5(b). It is observed that an increment in Reiner-Rivlin fluid parameters ϵ results in a temperature profile ϑξ . Fig. 5(c) illustrates the influence of Brownian motion. The larger the values of Brownian motion led to enhances the temperature profile ϑξ . The Brownian motion describes the erratic movement of nanoparticles embedded in a basic fluid as a result of contact with fluid molecules. Heat transportation theories, such as the Buongiorno nanofluid model, use the Brownian movement parameter Nb to quantify this. Fig. 5(d) signifies the mechanism of thermophoretic variable (Nt) against the temperature profile ϑξ . For increased values of Nt, the temperature field ϑξ is elevated. The thermal field ϑξ is exemplified in Fig. 5(e). The temperature profile ϑξ improves as the values of thermal radiation Rd increase has been elaborated in Fig. 5(f). In fact, the influence of conduction of surface heat transport values of Rd as a result of radiation, leading to an escalation in thermal field.

6.3 Concentration profile

The intensification in Brownian motion Nb leads to a decrease in Φξ has been explained in Fig. 6(a), respectively. As observed by Sabu et al. [35], an escalation in Brownian motion Nb fuels more collisions due to the haphazard motion of the nanoparticles; consequently, this causes an increase in temperature and a reduction in the volume fraction of the nanoparticles.

Fig 6(b) illustrates the thermophoretic force Nt acting across the nanoparticle concentration Φξ . The concentration Φξ displays a decrease as the values of Nt increase, as exemplified in Fig. 6(b). The thermophoretic force is generated by particles near the heated walls; this force causes an increase in temperature within the fluid region. The effects of the Schmidt number Sc on the concentration field Φξ have been illustrated in Fig. 6(c). In the case of higher Sc estimates, weaker concentrations are observed. The Schmidt number exhibits an inverse relationship with mass diffusivity. Therefore, elevated magnitude of Sc functioning to a reduction in mass diffusivity, which facilitates a more limited infusion of the solutal effect. As shown in Fig. 6(d), the weak mass diffusivity decreases concentration, while the stronger chemical reaction parameter Cr increases the reaction and consequently depreciates the concentration function Φξ .

6.4 Motile microorganism density

Fig. 7(a) displays the bioconvection Lewis number Lb changes the microbe field Υξ . When the bioconvection Lewis number Lb goes up, the microbe field goes down. Fig. 7(b) expressions the path of the Peclet number Pe on the microbe field. Higher Peclet number leads to reduced microbe field Υξ .

The effects of (M,λ) on friction factor, ( Ae,Sc) on mass rate and (Lb, Pe) on Nh are studied simultaneously using 3D surface plots, as shown in Figs. 8(a-d). According to Fig. 8(a), the drag is improved by the magnetic parameter M, and drag friction is at its peak for medium values of λ. The improved cross-viscosity causes the Reiner-Rivlin nanoliquid layers to rotate, which in turn causes strains across velocity gradients. Fig. 8(c) shows that, unlike the activation energy parameter Ae , which decreases as the mass rate increases with the nanoparticle volume Sc. The Lb jump enhances microorganisms in the nano liquid. The microorganisms decrease as the Pe increases, as predicted by the physical phenomenon seen in Fig. 8(d).

Grid sketch for the axial velocity Fξ , radial velocity F ξ , azimuthal velocity Gξ , temperature profile ϑξ , concentration field Φξ and density profile Υξ has been revealed in Figs. 9(a-f).

The numerical results for drag friction, azimuthal velocity, axial velocity, and radial velocity have been presented in Table 3. These results pertain to different mixed convective variable γ and the Reiner-Rivlin parameters λ. In this case, the volumetric flow rate of the von Karman problem is assisted by F(). Using G'(0), the driving torque or disk torque is measured. As a result of the viscoelastic impacts, the Von Karman flow torque is altered. Resisting torque and the coefficient of surface drag force increase as the radial and tangential velocity components increase in magnitude. As the tangential slip parameter increases, it is understood that the torque at the disk increases. Furthermore, an analysis of the tabulator magnitudes reveals that both the skin friction coefficient and driving torque exhibit a progressive trend with respect to the Reiner–Rivlin parameter. Conversely, a contrary pattern is observed with regard to the heat rate for the greater values of Rd, Nb, and Nt has been mentioned in Table 4. The mass flux rate for distinct values of Sc, Cr, Ae have been illustrated in Table 5. The rate of mass enhances for high values of Sc, Cr, while the opposite is true for Ae . Table 6 presents a variety of local density profile estimations for Pe and Lbat varying values. As the values of Lb, and Pe increase, the local density of microorganisms is observed to rise, whereas it decreases as the parameter increases. Table 7 represents the analysis of ξ for the different values of Fξ ,  F'ξ , Gξ , ϑξ , Φξ, and Υξ .

Table 3. Calculation of F(), F(0), G(0) wall stress along with skin friction while other parameters are Rd=0.1,Nb=0.2,Nt=0.1,Q=0.1,Sc=0.6,Cr=0.1 JK966_268 - Copy.eps] Λ=0.9,n=0.5, Ae=0.1,Lb=0.2,Pe=0.4,ω=0.1, β1 =0.2, β2 =0.2, γ1 =0.3, γ2 =0.3.
λ γ Nr Nc M F() F’’(0) G’(0) (F’’(0)) 2 + (G’(0)) 2
0.5 0.1 0.1 0.2 0.2 0.5882 0.2721 -0.7380 0.7866
0.6 0.5779 0.2527 -0.7409 0.7828
0.7 0.5673 0.2329 -0.7413 0.7770
0.8 0.5565 0.2128 -0.7393 0.7693
0.4 0.3 0.9794 0.3831 -0.8587 0.9403
0.5 1.2413 0.4861 -0.9740 1.0886
0.7 1.4459 0.5953 -1.0840 1.2367
0.9 1.6157 0.7096 -1.1922 1.3874
0.2 0.3 0.7874 0.3166 -0.7791 0.8410
0.4 0.7747 0.3074 -0.7697 0.8289
0.5 0.7614 0.2983 -0.7602 0.8166
0.6 0.7476 0.2892 -0.7505 0.8043
0.2 0.3 0.7966 0.3158 -0.7791 0.8407
0.4 0.7930 0.3059 -0.7698 0.8283
0.5 0.7891 0.2961 -0.7603 0.8159
0.6 0.7846 0.2863 -0.7508 0.8035
0.1 0.6 0.6152 0.2434 -0.8728 0.9061
0.8 0.5386 0.2079 -0.9146 0.9379
1 0.4737 0.1781 -0.9568 0.9732
1.2 0.4193 0.1531 -0.9985 1.0101
Table 4. Calculation of ϑ'(0) while other parameters are λ=0.5, γ=0.3, Nr=0.1, Nc=0.2, JK966_279 - Copy.eps] M=0.3,Sc=0.6, Cr=0.1, Λ=0.9,n=0.5,Ae=0.1, Lb=0.2, Pe=0.4, ω=0.1,β1 =0.2,  β2 =0.2, γ1 =0.3, γ2 =0.3.
Rd Pr Nb Nt Q Nu
0.1 0.7 0.1 0.3 0.1 0.1933
0.2 0.2115
0.3 0.2293
0.4 0.2469
0.3 0.2604
0.5 0.2496
0.7 0.2385
0.9 0.2275
0.2 0.2 0.2705
0.4 0.2597
0.6 0.2493
0.8 0.2395
0.1 0.1 0.2 0.1332
0.3 0.1093
0.4 0.0834
0.5 0.0551
Table 5. Calculation of Φ(0) while other parameters are λ=0.5,γ=0.3,Nr=0.1,Nc=0.2,JK966_287 - Copy.eps] M=0.3,Rd=0.1,Nb=0.1,Nt=0.3,Q=0.1,n=0.5,Lb=0.2,Pe=0.4,ω=0.1, β1 =0.2, β2 =0.2, γ1 =0.3, γ2 =0.3.
Sc Cr Λ Ae Sh
0.3 0.3 0.2 0.1 0.2655
0.4 0.3244
0.5 0.3746
0.6 0.4180
0.2 0.3565
0.4 0.4699
0.6 0.5541
0.8 0.6213
0.1 0.3 0.2836
0.5 0.2887
0.7 0.2935
0.9 0.2979
1.2 0.2443
1.4 0.2375
1.6 0.2314
1.8 0.2260
Table 6. Calculation of Υ(0) Motile transfer rate while other parameters are as λ=0.5,γ=0.3,Nr=0.1,Nc=0.2,M=0.3,Rd=0.1,Nb=0.1,Nt=0.3,Q=0.1,Sc=0.3, Cr=0.3,Λ=0.2,n=0.5, Ae=0.1, β1 =0.2, β2 =0.2, γ1 =0.3, γ2 =0.3
Lb Pe ω Nh
0.3 0.2 0.1 0.3630
0.4 0.3970
0.5 0.4281
0.6 0.4566
0.2 0.3 0.3916
0.5 0.5227
0.7 0.6550
0.9 0.7886
0.4 0.2 0.6232
0.3 0.7877
0.4 0.9507
0.5 1.1122
Table 7. Grid sensitivity analysis when λ=0.1,γ=0.1,Nr=0.1,Nc=0.1,M=0.4,Rd=0.1,JK966_299 - Copy.eps] Nb=0.2,Nt=0.1,Q=0.1,Sc=0.6,Cr=0.1,Λ=0.9,n=0.5, Ae=0.1,Lb=0.2,Pe=0.4, ω=0.1, β1 =0.2, β2 =0.2, γ1 =0.3, γ2 =0.3.
Function Step size ξ
1 2 4 6 8
Fξ 50 0.1281 0.2623 0.4354 0.5152 0.5339
100 0.1281 0.2623 0.4354 0.5152 0.5339
150 0.1281 0.2623 0.4354 0.5152 0.5339
F ξ 50 0.1483 0.1170 0.0603 0.0219 0
100 0.1483 0.1170 0.0603 0.0219 0
150 0.1483 0.1170 0.0603 0.0219 0
Gξ 50 0.3174 0.1040 0.0085 0.0006 0
100 0.3174 0.1040 0.0085 0.0006 0
150 0.3174 0.1040 0.0085 0.0006 0
ϑξ 50 0.8381 0.7073 0.4470 0.2074 0
100 0.8381 0.7073 0.4470 0.2074 0
150 0.8381 0.7073 0.4470 0.2074 0
Φξ 50 0.5745 0.3422 0.1050 0.0283 0
100 0.5745 0.3422 0.1050 0.0283 0
150 0.5745 0.3422 0.1050 0.0283 0
Υξ 50 0.5981 0.3117 -0.0017 -0.0786 0
100 0.5981 0.3117 -0.0017 -0.0786 0
150 0.5981 0.3117 -0.0017 -0.0786 0

7. Future Scope

This study presents a detailed analysis of Reiner-Rivlin nanofluid flow with gyrotactic microorganisms over a rotating disk under multiple slip conditions. Future research could explore unsteady and 3D flow to capture transient and realistic dynamics. Incorporating external electric, magnetic, or thermal effects would enhance the model’s relevance to advanced fluid applications. Investigating hybrid nanofluids and varying nanoparticle shapes may improve heat and mass transfer predictions. Bioconvective stability analysis can deepen understanding of microorganism-induced patterns. Finally, experimental and CFD-based validation would strengthen the model’s practical applicability in biomedical and industrial systems.

8. Conclusions

The explanation connects with the gyrotactic microorganism on Reiner-Rivlin nano liquid and activation energy aspects past a disk in rotatory flow through slip effect and thermal solutal convective condition. The converted ODEs are numerically solved by Bvp4c. The effects of various variables have been deliberated in graphical form. The major point of this analysis is highlighted below.

  • When the Reiner Rivlin variables change, the radial flow outside the disk slows down. This reduced flow is then improved by centrifugal force.

  • Wall slip parameter rises result in a reduction in radial velocity.

  • The radial velocity profile goes up as the convective variable goes up.

  • As the Brownian motion parameter and radiation parameter enhance, so does the rate of heat movement accelerate.

  • When Sc and Cr values upturn, concentration goes down.

  • With an increase in Pe and Lb, the motile density profile exhibits a declining trend.

Acknowledgement

Princess Nourah bint Abdulrahman University Researchers Supporting Project number (PNURSP2025R920), Princess Nourah bint Abdulrahman University, Riyadh, Saudi Arabia. The authors also extend their appreciation to Northern Border University, Saudi Arabia, for supporting this work through project number (NBU-CRP-2025-2484).

CRediT authorship contribution statement

Essam R. El-Zahar: Conceptualization, methodology; Syed Shoaib Zafar: Visualization, investigation, supervision; Talha Anwar: Validation, supervision, formal analysis, writing – original draft preparation; Khalid S. Almutairi: Methodology, software; Habib Kraiem: Formal analysis, investigation, writing – original draft preparation; Farhan Ali: Conceptualization, validation, writing – review & editing, M. Faizan: Software, writing – review & editing; Asra Anjum: Methodology, writing – review & editing.

Declaration of competing interest

The authors declare that they have no competing financial interests or personal relationships that could have influenced the work presented in this paper.

Data availability

All data used in this manuscript have been presented within the article.

Use of artificial intelligence (AI)-assisted technology for manuscript preparation

The authors confirm that there was no use of AI-assisted technology for assisting in the writing of the manuscript and no images were manipulated using AI.

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