Optical and structural properties of TaC thin films: Towards design of an efficient high temperature solar absorber coating

• TaC thin films prepared by Pulsed DC sputtering from Ta target in C2H2 + Ar atmosphere. • Phase formation of TaC confirmed by XRD and XPS in limited C2H2 flow range. • Comprehensive refractive index analysis of TaC films from 300 nm to 1700 nm. • Validated optical models accurately simulate SSA performance across wide spectra. • High-temperature solar absorber with > 80 % efficiency for CSP systems at 1200 °C. Tantalum and Tantalum Carbide (TaC) thin films are fabricated using pulsed DC magnetron sputtering from a Ta target in an argon-acetylene (C 2 H 2 ) environment at room temperature. Precise control of the TaC x film composition was achieved, with minimal impact on the films’ structure, morphology, and optical properties observed when varying C 2 H 2 gas concentrations, ensuring high reproducibility rate. Ellipsometry analysis determined the complex refractive index of the TaCx films, enabling accurate reproduction of reflectivity spectra in both visible and infrared regions. As the knowledge of the refractive index is crucial for simulating optical structures, an optimised selective solar absorber (SSA) for use in concentrating solar-thermal power (CSP) systems was designed. It comprises TaC and SiN layers on a tungsten substrate; hence, it is capable of withstanding high temperatures. It has a solar absorptance of 0.96 and a thermal efficiency higher than 0.9 at 900 °C and 0.85 at 1100 °C for incident angles up to 50 °C for a concentration factor of 1000. Its large acceptance angle offers significant potential for energy production through heliostats where the incident angle may vary.

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Publication Details

Journal
Solar Energy
Published
2025-03-29
DOI
https://doi.org/10.1016/j.solener.2025.113459
Citations
2
Primary Topic
Solar Thermal and Photovoltaic Systems
Type
article
Field-Weighted Citation Impact
0.73
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article

Optical and structural properties of TaC thin films: Towards design of an efficient high temperature solar absorber coating

R. Russo, Antonio Caldarelli, Harish C. Barshilia, Daniela De Luca et al.
2 citations
Solar Energy
Solar Thermal and Photovoltaic Systems
0.73
article

Optical and structural properties of TaC thin films: Towards design of an efficient high temperature solar absorber coating

R. Russo, Antonio Caldarelli, Harish C. Barshilia, Daniela De Luca, Parthasarathi Bera, Tejal Chandrakant Gawade
article en
2 citations

Abstract

• TaC thin films prepared by Pulsed DC sputtering from Ta target in C2H2 + Ar atmosphere. • Phase formation of TaC confirmed by XRD and XPS in limited C2H2 flow range. • Comprehensive refractive index analysis of TaC films from 300 nm to 1700 nm. • Validated optical models accurately simulate SSA performance across wide spectra. • High-temperature solar absorber with > 80 % efficiency for CSP systems at 1200 °C. Tantalum and Tantalum Carbide (TaC) thin films are fabricated using pulsed DC magnetron sputtering from a Ta target in an argon-acetylene (C 2 H 2 ) environment at room temperature. Precise control of the TaC x film composition was achieved, with minimal impact on the films’ structure, morphology, and optical properties observed when varying C 2 H 2 gas concentrations, ensuring high reproducibility rate. Ellipsometry analysis determined the complex refractive index of the TaCx films, enabling accurate reproduction of reflectivity spectra in both visible and infrared regions. As the knowledge of the refractive index is crucial for simulating optical structures, an optimised selective solar absorber (SSA) for use in concentrating solar-thermal power (CSP) systems was designed. It comprises TaC and SiN layers on a tungsten substrate; hence, it is capable of withstanding high temperatures. It has a solar absorptance of 0.96 and a thermal efficiency higher than 0.9 at 900 °C and 0.85 at 1100 °C for incident angles up to 50 °C for a concentration factor of 1000. Its large acceptance angle offers significant potential for energy production through heliostats where the incident angle may vary.

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