Solar energy improvement in solar HVAC using Sutterby magneto‐ternary hybrid nanofluid flow with Smoluchowski temperature conditions: A solar thermal application

Abstract

Abstract This study investigates the radiative flow of rotating Sutterby magneto‐ternary hybrid nanofluids traveling along a stretchy surface in solar heating, ventilation, and air conditioning (HVAC). The investigation includes a colloidal mixture of three district types of particles, and impacts such as thermal radiative fluxing and activation energy. This model is used for the Sutterby model, and the flow and heat transfer analysis developed the new idea of tri‐hybrid nanofluid for highlighting some unique thermal properties in the fluid flow problems. The tri‐hybrid nanofluid is formed by suspending the three different nanoparticles for advanced cooling purposes. In the present work, we have considered Molybdenum disulfide (MoS2), Graphene oxide (GO), and Multi‐walled carbon nanotubes (MCNT) in water for advanced cooling. The study uses the Runge‐Kutta‐Fehlberg method to simulate the system and analyzes physical attributes such as skin friction coefficient and Nusselt and Sherwood numbers. The results suggest that increasing activation energy leads to an increase in the concentration of nanoparticles, and increasing rotational parameters leads to an increase in radial skin friction but a decrease in Nusselt numbers. The study also found that ternary nanofluids are more effective than base fluids in enhancing convective heat and mass transfer

Topics & Concepts