Solar system physical treatment using a turbulator and nanomaterial through absorber duct

A three-part tape-enhanced tube was used in the current hypothetical solar unit to save the most radiation possible. The three parts were joined at different angles (beta). The parameters of the carrier base fluid after mixing with CuO nanopowder were calculated using a homogeneous model. By adjusting the range of Y+, multiple layers were used to precisely depict the behavior of flow close to the wall. The results show the components of irreversibility as bar charts, velocity contours, and exergy drop contours. The tape angle (beta) and inlet velocity were thought to be the main driving forces. An evaluation of the accommodation's validity using numerical data shows that it is sufficient. The wall temperature decreases by about 0.0257% as the nanofluid angle rises and more collisions with the wall take place. Xd falls off roughly 5.19% from 0(degrees) to 45(degrees) and 5.87% from 0(degrees) to 90(degrees) as the angle beta rises. As beta rises, the entropy of friction increases by 9.88%. The outer wall cools by about 0.87% and Xd falls by about 92.3% when beta=45 degrees and Re rises.