Analyzing the Raman Spectra of Graphenic Carbon Materials from Kerogens to Nanotubes: What Type of Information Can Be Extracted from Defect Bands?
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carbon-05-00069-v2.pdf
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385ef91269f5f91d7f97cf4167f55334
Author(s) • • • • • • • • •
Puech, Pascal
Kandara, Mariem
Paredes, Germercy
Moulin, Ludovic
Weiss-Hortala, Elsa
Kundu, Anirban
Ratel-Ramond, Nicolas
Plewa, Jérémie-Marie
Pellenq, Roland
Monthioux, Marc
Date Issued
November 2019
Journal
C: Journal of Carbon Research
Publisher
MDPI
Citation
Puech, Pascal et al. "Analyzing the Raman Spectra of Graphenic Carbon Materials from Kerogens to Nanotubes: What Type of Information Can Be Extracted from Defect Bands?" C: Journal of Carbon Research 5, 4 (November 2019): 69 © 2019 The Author(s)
Version
Final published version
Abstract
Considering typical spectra of a broad range of carbonaceous materials from gas-shale to nanotubes, various ways by which defects show up in Raman spectra are exampled and discussed. The position, resonance behavior, and linewidth of both the D and G bands are compared, even if in some cases obtaining accurate information on the materials from the fitting parameters is a difficult task. As a matter of fact, even if a full picture is unreachable, defining parameter trends is one acceptable option. Two ways to determine the linewidth, either graphically and or by fitting are proposed in order to be able to compare literature data. The relationship between the crystallite size obtained from the linewidth and from X-ray diffraction, which is complementary to the Tuinstra and Koenig law, is examined. We show that a single approach is not possible unless modeling is performed and therefore that analysis of Raman spectra should be adapted to the specificities of each sample series, i.e., a minimum of knowledge about the materials is always required.
MIT Department
Massachusetts Institute of Technology. Department of Materials Science and Engineering
Terms of Use
Creative Commons Attribution 4.0 International license
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DOI of Published Version
https://doi.org/10.3390/c5040069