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DSMC Simulation of Etch Pit Formation Through Active Sites in Carbon Fiber Micro-StructuresErosion of carbon due to oxidation does not occur uniformly but through localized etch pit formation because of active surface sites. In this work we demonstrate a newly developed capability to capture pitting of carbon fiber microstructures such as FiberForm, which is commonly used as the base material for NASA’s spacecraft ablative thermal protection systems (TPS). The simulations are performed at the meso-scale in order to capture the pit formation and growth using direct simulation Monte Carlo (DSMC), specifically using the Stochastic PArallel Rarefied-gas Time-accurate Analyzer (SPARTA) code. Legacy and latest models both assume uniform reactivity of carbon surface sites with oxygen even at the meso-scale level. However, in reality the carbon surface has locally different reaction rates due to the presence of defects at the atomic scale. The defective nature of these sites enhances their reactivity with atmospheric gases compared to the non-defective sites (2-3 orders of magnitude) and are termed as “active sites”. Thus, these sites tend to be the first to react and eventually get removed through the formation of gases such as CO, CO2, and CN. Their removal results in all the neighboring atoms becoming defective, thus leading to chain reaction of localized carbon removal and formation of etch pits. Capturing the formation of pits during the ablation simulation of carbon micro-structures is critical to predicting their structural failure. Recently a detailed surface chemistry framework was developed in SPARTA, capable of incorporating various detailed surface reaction mechanisms. We have implemented the capability of a single surface having multiple site sets with different reactivities within this framework. We have used this feature to model the presence of active sites on carbon surfaces, whose reactivity is orders of magnitude higher than that of the passive sites due to the presence of defects. The active site fraction is a property of surface elements within SPARTA and is directly proportional to the local reactivity of each surface element. By introducing an initial distribution of the active site fraction across the carbon surface and propagating it in a manner that mimics the evolution of real reacting carbon surfaces, we can capture the formation and growth of etch pits as a result of surface consumption reactions such as oxidation.
Document ID
20230013518
Acquisition Source
Ames Research Center
Document Type
Presentation
Authors
Krishnan Swaminathan Gopalan
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Simon Schmitt
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Arnaud Borner
(Analytical Mechanics Associates (United States) Hampton, Virginia, United States)
Date Acquired
September 18, 2023
Subject Category
Chemistry and Materials (General)
Composite Materials
Meeting Information
Meeting: Direct Simulation Monte Carlo (DSMC) Conference 2023
Location: Santa Fe, NM
Country: US
Start Date: September 24, 2023
End Date: September 27, 2023
Sponsors: Sandia National Laboratories
Funding Number(s)
CONTRACT_GRANT: NNA15BB15C
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
Keywords
DSMC
Microstructure
Carbon
Pitting
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