ATOMIC AND MICROSTRUCTURAL ORIGINS OF STORED ENERGY RELEASE IN NEUTRON-IRRADIATED SILICON CARBIDE
Here, we employ a combination of advanced synchrotron-based scattering characterization techniques to understand and unravel the atomic origins of the colossal stored energy release in neutron irradiated silicon carbide. The quantification of the neutron irradiation-induced defects, and their impact on the structureproperty relationship is important for the design and safe operation of advanced fission and fusion reactors. Our experimental results show that the atomic structure in the as irradiated samples is significantly perturbed due to a large fraction of vacancy and interstitial type defects that lead to complex microstructures and additional components in the x-ray diffraction and pair distribution function results. We directly correlate the stored energy release to the recovery of the sub-lattices, with pair distribution function analysis highlighting that the carbon interstitial and vacancy-type defects contribute to stored energy more than those of silicon. We find these results to be striking and believe our discoveries to be timely and noteworthy given the technological importance of silicon carbide to the nuclear fission and fusion communities.
- Research Organization:
- Nuclear Science User Facilities
- Sponsoring Organization:
- Nuclear Science User Facilities
- DOE Contract Number:
- AC07-05ID14517;
- OSTI ID:
- 3021722
- Country of Publication:
- United States
- Language:
- English
Similar Records
Atomic and microstructural origins of stored energy release in neutron-irradiated silicon carbide
Stored energy in irradiated silicon carbide
Using defects to store energy in materials – a computational study
Journal Article
·
Thu Oct 07 20:00:00 EDT 2021
· Physical Review Materials
·
OSTI ID:1826005
Stored energy in irradiated silicon carbide
Technical Report
·
Mon Mar 31 23:00:00 EST 1997
·
OSTI ID:543282
Using defects to store energy in materials – a computational study
Journal Article
·
Mon Jun 12 20:00:00 EDT 2017
· Scientific Reports
·
OSTI ID:1490407