Insights into the 3D Slip Dynamics of Jeffrey Fluid Due to a Rotating Disk with Exponential Space-Dependent Heat Generation: A Case Involving a Non-Fourier Heat Flux Model

The dynamics of non-Newtonian Jeffrey fluid in conjunction with a spinning disk surface can be problematic heating systems, polymer technology, microelectronics, advanced and substantive disciplines. Therefore, the significance Hall current Coriolis forces terms flowing across gyrating subject to non-Fourier heat flux was investigated this study. A temperature-related source (TRHS) exponential-related (ERHS) were incorporated into model improve thermal characteristics. Thermal radiation multiple slip effects employed flow system. connected non-linear PDEs governing transport transmuted ODEs solved using Runge–Kutta shooting technique (RKST). results RKST substantiated previous studies found have adequate reliability. numerical values coefficient friction Nusselt number simulated. higher rate transfer (HTR) than traditional Fourier flux. Furthermore, both TRHS ERHS phenomena support progression HTR. swelling influence velocities, whilst temperature shows opposite tendency. asymptotic variances detected for larger parameter values.