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Title: A review of cermet-based spectrally selective solar absorbers

Journal Article · · Energy & Environmental Science
DOI:https://doi.org/10.1039/c3ee43825b· OSTI ID:1384135
 [1];  [2];  [2];  [1]
  1. Univ. of Houston, TX (United States)
  2. Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)

Spectrally selective solar absorbers harvest solar energy in the form of heat. Solar absorbers using cermet-based coatings reflect a high absorptance of the solar spectrum and a low emittance in the infrared (IR) regime. Extensive work has been done to optimize cermet-based solar absorbers to achieve high performance by exploring different cermet (ceramic–metal composite) materials and film configurations through different preparation techniques such as electrodeposition, sputtering, pulsed laser deposition, and solution-based methods. Here in this work, we review the progress of cermet-based spectrally selective absorbers with high solar absorptance and low thermal emittance, such as Cr2O3, Al2O3, AlN, SiO2, and ZrO2 based cermets as absorption layers. We also present an outlook for cermet-based spectrally selective absorbers with high thermal stability and high conversion efficiency from sunlight to heat.

Research Organization:
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Energy Efficiency and Renewable Energy (EERE), Renewable Power Office. Solar Energy Technologies Office
Grant/Contract Number:
SC0001299; FG02-09ER46577; EE0005806
OSTI ID:
1384135
Journal Information:
Energy & Environmental Science, Vol. 7, Issue 5; Related Information: S3TEC partners with Massachusetts Institute of Technology (lead); Boston College; Oak Ridge National Laboratory; Rensselaer Polytechnic Institute; ISSN 1754-5692
Publisher:
Royal Society of ChemistryCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 355 works
Citation information provided by
Web of Science

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