Lifetime modeling for a supercritical CO2-molten salt CSP power block

Bruce A. Pint, Stephen S. Raiman, James R. Keiser

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

2 Scopus citations

Abstract

To achieve higher efficiency in the next generation of concentrating solar power (CSP) plants, higher temperatures are needed, which will challenge the materials. One scenario would include molten chloride salts for thermal storage and supercritical CO2 (sCO2) for the power block and operating temperatures above 700°C to achieve at least 50% efficiency. For the high pressure (20-30MPa) sCO2 conditions, high strength Ni-based alloys will be required above 700°C and an extensive experimental project has confirmed good sCO2 compatibility for alloys 625, 740H and 282. The data set generated enables more accurate lifetime predictions for 30-year service. Compatibility testing with K-Mg-Na chloride salts has just begun. Initial isothermal capsule results indicate there are promising combinations of salt chemistry, temperature and alloy composition. However, flowing salt testing is needed to evaluate compatibility, which is in progress.

Original languageEnglish
Title of host publicationSolarPACES 2018
Subtitle of host publicationInternational Conference on Concentrating Solar Power and Chemical Energy Systems
EditorsChristoph Richter
PublisherAmerican Institute of Physics Inc.
ISBN (Electronic)9780735418660
DOIs
StatePublished - Jul 25 2019
Event24th SolarPACES International Conference on Concentrating Solar Power and Chemical Energy Systems, SolarPACES 2018 - Casablanca, Morocco
Duration: Oct 2 2018Oct 5 2018

Publication series

NameAIP Conference Proceedings
Volume2126
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

Conference24th SolarPACES International Conference on Concentrating Solar Power and Chemical Energy Systems, SolarPACES 2018
Country/TerritoryMorocco
CityCasablanca
Period10/2/1810/5/18

Funding

The authors would like to thank M. Howell, A. Willoughby, M. Stephens, G. Garner, T. Lowe, T. Jordan, H. Meyer, D. Leonard, M. Lance, R. Mayes and J. Kurley at ORNL and S. Pearson from Akron U. for assistance with the experimental work and the other members of our research team: Brayton Energy, LLC, Special Metals, Haynes International and Sandvik and the input of others from the CSP/sCO2 industry. This research was funded by the SunShot Initiative under the U.S. Department of Energy's Office of Energy Efficiency and Renewable Energy, Solar Energy Technology Program: SuNLaMP award number DE-EE0001556 and CSP award number 33873 The authors would like to thank M. Howell, A. Willoughby, M. Stephens, G. Garner, T. Lowe, T. Jordan, H. Meyer, D. Leonard, M. Lance, R. Mayes and J. Kurley at ORNL and S. Pearson from Akron U. for assistance with the experimental work and the other members of our research team: Brayton Energy, LLC, Special Metals, Haynes International and Sandvik and the input of others from the CSP/sCO2 industry. This research was funded by the SunShot Initiative under the U.S. Department of Energy’s Office of Energy Efficiency and Renewable Energy, Solar Energy Technology Program: SuNLaMP award number DE-EE0001556 and CSP award number 33873.

FundersFunder number
Haynes International and Sandvik
U.S. Department of Energy
Solar Energy Technologies Program33873, DE-EE0001556
Office of Energy Efficiency and Renewable Energy
Oak Ridge National Laboratory

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