## 5 Comprehensive Debate Based on Numerical Results  
This segment has been launched to discuss the impact of several physical factors on the rapidity, temperature, and concentricity outlines. The engineering amounts of attention  
Figure 2: Flow chart of Lobatto IIIA scheme. such as the frictional force and Nusselt quantity were calculated and portrayed in the form of figures and tables. Figure 3 is constructed to study the effect of unsteadiness parameter \(A\) on the rapidity field in the absence (presence) of an inclination angle. It is quite evident that amplification in the unsteadiness parameter brings about an increment change in the fluid velocity. The inclination angle magnifies due to magnification in \(A\), which escalates the fluid flow and the velocity field. The effect of the Grashof number \(G\) on the velocity field in the absence (presence) of the inclined angle \(\omega\) is highlighted in Figure 4. The Grashof number is the ratio of buoyancy forces to the viscous forces. A positive change in \(G\) intensifies the buoyancy forces instead of viscous forces. The density of the fluid diminishes owing to an enrichment in \(G\), which lessens the fluid viscosity and magnifies the fluid velocity. The velocity of fluid diminishes by the virtue of magnification in the power-law index \(n\) as shown in Figure 5. The parameter \(n\) decides how viscous the fluid is. Fluid behavior in the case of \(n<1\) is shear thinning, \(n=1\) is Newtonian, and \(n>1\) is shear thickening. The fluid becomes much dense, and viscosity amplifies due to an increase in \(n\) which brings about an abatement in \(f^{\prime}(\eta)\). An incremental change in electrical conductivity allows more current to flow through the fluid which creates a resistive force termed Lorentz force, which depreciate the fluid motion and furthermore diminish \(f^{\prime}(\eta)\) as shown in Figure 6. Figure 7 reveals the influence of the Weissenberg number \(We\) on \(f^{\prime}(\eta)\). The parameter We represents the relaxation time, the time in which the fluid deforms to regain its original shape. During that time the viscosity of the fluid increases, which depreciates the fluid velocity. The Weissenberg number is the ratio of elastic forces to viscous forces. The fluid becomes more viscous by escalating \(We\) which lessens the fluid motion and \(f^{\prime}(\eta)\). The heat transfer coefficient \(\gamma\) is determined by the transfer of heat from one place to another and the heat transfer rate amplifies on the behalf of magnification in \(\gamma\) as shown in Figure 8. It is observed that the rate of convective heat transfer is proportional to the temperature difference. A positive variation in \(\gamma\) provides substantial heat which is absorbed by the system and amplifies the temperature field. Radiation is one of the modes of heat transfer, with the other two being conduction and convection. Nonlinear thermal radiation is employed where the elevated temperature change is required and has immense utilization in an industry such as polymer fabrication, combusting apparatuses, satellites, etc. Thermal radiation is directly related to the temperature difference. The temperature of the fluid escalates because of a positive change \(N\) which enhances the temperature field \(\theta(\eta)\) as shown in Figure 9. Figure 10 investigates the impact of the Prandtl number on \(\theta(\eta)\). The Prandtl number is a ratio of momentum diffusivity to thermal diffusivity. It is observed that the thermal diffusivity of nanoparticles lessens because of magnification of the Prandtl number \(Pr\), which depreciates the temperature of the fluid and heat transfer rate. From Figure 11 it is observed that the temperature field amplifies owing to amplification in \(\theta_{w}\). The parameter \(\theta_{w}\) is an important part of nonlinear thermal radiation along with \(N\).