In this study, two planar high-temperature solar receivers, equipped with Triply Periodic Minimal Surface lattices of Diamond and SplitP, were analysed numerically. These receivers were manufactured and experimentally tested in a previous study. Different RANS turbulence models, including Lag EB κ-ε, κ-ω SST (Menter), and Realizable κ-ε two-layer, were evaluated, and their results were compared with experimental data. A comprehensive validation revealed that the Lag EB κ-ε and κ-ω SST (Menter) models have the smallest deviation from the experimental data. The sample with the SplitP lattice demonstrated superior thermal performance with higher thermal efficiency, higher useful heat, and exhibiting a slightly lower maximum surface temperature and a narrower high-temperature region.

Numerical Modelling of Solar Receivers Equipped With TPMS Structures / Mortazavi, Arsham; Ebadi, Hossein; Piatti, Cecilia; Gajetti, Eleonora; Marocco, Luca; Savoldi, Laura. - 3:(2025). ( SolarPACES 2024, 30th International Conference on Concentrating Solar Power, Thermal, and Chemical Energy Systems) [10.52825/solarpaces.v3i].

Numerical Modelling of Solar Receivers Equipped With TPMS Structures

Mortazavi, Arsham;Ebadi, Hossein;Piatti, Cecilia;Gajetti, Eleonora;Marocco, Luca;Savoldi, Laura
2025

Abstract

In this study, two planar high-temperature solar receivers, equipped with Triply Periodic Minimal Surface lattices of Diamond and SplitP, were analysed numerically. These receivers were manufactured and experimentally tested in a previous study. Different RANS turbulence models, including Lag EB κ-ε, κ-ω SST (Menter), and Realizable κ-ε two-layer, were evaluated, and their results were compared with experimental data. A comprehensive validation revealed that the Lag EB κ-ε and κ-ω SST (Menter) models have the smallest deviation from the experimental data. The sample with the SplitP lattice demonstrated superior thermal performance with higher thermal efficiency, higher useful heat, and exhibiting a slightly lower maximum surface temperature and a narrower high-temperature region.
2025
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11583/3005668