4.6 Article

Tungsten nanopore-based near-ideal spectral selective solar absorber for a wide temperature range

Journal

SOLAR ENERGY
Volume 248, Issue -, Pages 149-159

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.solener.2022.11.003

Keywords

Solar energy; Solar selective absorber; High efficiency; Regular hexagonal nanopore; Wide temperature range

Categories

Funding

  1. National Natural Science Foundation of China
  2. Natural Science Foundation of Hunan Province
  3. Central South Univer-sity Innovation-Driven Research Programme
  4. [52006247]
  5. [52176093]
  6. [2021JJ40753]
  7. [2023CXQD056]

Ask authors/readers for more resources

In this study, a simple and efficient spectral selective solar absorber consisting of hexagonal tungsten nanopores filled with silicon dioxide was proposed. The absorber exhibited high solar absorptivity and low total emissivity, and achieved high photothermal efficiencies at different concentrations. Mechanism analysis revealed that the excellent performance of the absorber was attributed to the enhanced electromagnetic field, localized surface plasmon resonances, and impedance matching. Furthermore, the absorber showed insensitivity to incident angle and polarization angle, and was applicable to different waveguide modes.
An efficient and simple spectral selective solar absorber is vital for solar-thermal systems that operate under a wide temperature range (673-1573 K). However, few absorbers are competent for this wide temperature range due to their suboptimal spectral selectivity under specific conditions or complex structures that are difficult to be fabricated. Here, we proposed a near-ideal spectral selective solar absorber consisting of simple regular hexag-onal tungsten nanopores filled with silicon dioxide. A strong solar absorptivity up to 0.9632 and a reduced total emissivity down to 0.0961 were realized due to its good spectral selectivity. Meanwhile, the near-ideal spectral selective solar absorber obtains high photothermal efficiencies of 95.25 % at 673 K, 95.84 % at 873 K, and 89.38 % at 1573 K when the concentration ratios are 100, 1000, and 2000 suns, respectively. Subsequently, mechanism analysis implies that the excellent performance of the near-ideal absorber results from the electromagnetic field enhanced by the cavity resonances, localized surface plasmon resonances, and surface plasmon polaritons. Further, the impedance matching also plays an important role in achieving the excellent performance. In addition, the near-ideal absorber also shows insensitivity to incident angle and polarization angle with both TE and TM waves. All the above positive properties presented by the near-ideal absorber indicate that it is a good option for solar energy capture in the wide temperature range of 673-1573 K.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available