Real time observation of glass-like carbon formation from SU-8 using X-ray and ultraviolet photoelectron spectroscopy

The structural development and change in elemental composition of SU-8 3005 photoresist into glass-like carbon due to pyrolysis up to 1000 ° C is investigated utilising in-situ x-ray and ultraviolet photoelectron spectroscopy (XPS/UPS) under ultra-high vacuum (UHV). XPS spectra were analysed in order to investigate changes to elemental composition and physical structure. Peak asymmetry in the measured C 1s spectra is found to be a clear indicator of a transition in both physical structure and increased electrical conductivity. The in-situ XPS measurement of pyrolysis is effective in isolating changes in oxygen composition solely due to the pyrolysis process. Oxygen concentration, C 1s peak asymmetry and C 1s peak positions are strong indicators of semiconducting SU-8 transitioning to conducting glass-like carbon. For SU-8 pyrolysed above temperatures of 500 ° C, a clear development is observed in the material structure and composition towards a carbon rich conducting network indicative of glass-like carbon. UPS spectra were analysed to investigate the changes in secondary electron cut-off (SECO) and valence band maximum (VBM) as the SU-8 layer is heated in UHV. The changes in SECO and VBM correlates well with the XPS data and a zero binding energy state is observed at 1000 ° C. • In-situ observation of glass-like carbon formation. • X-ray photoelectron spectroscopy showing transformation of non - conductive SU-8 to a conductive thin film. • Observation of structural oxygen reduction between 300 and 600 °C leading to the formation of a carbon rich network. • Appearance of various features in UPS data in-line with compositional changes observed in XPS data. • Appearance of zero binding energy state at 1000 ° C.

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Publication Details

Journal
Carbon
Published
2025-08-22
DOI
https://doi.org/10.1016/j.carbon.2025.120728
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00

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article

Real time observation of glass-like carbon formation from SU-8 using X-ray and ultraviolet photoelectron spectroscopy

Simon Astley, D. A. Evans, Jerome A. Cuenca, Oliver A. Williams et al.
Carbon
Astro and Planetary Science
article

Real time observation of glass-like carbon formation from SU-8 using X-ray and ultraviolet photoelectron spectroscopy

Simon Astley, D. A. Evans, Jerome A. Cuenca, Oliver A. Williams, Soumen Mandal, Jaspa Stritt
article en

Abstract

The structural development and change in elemental composition of SU-8 3005 photoresist into glass-like carbon due to pyrolysis up to 1000 ° C is investigated utilising in-situ x-ray and ultraviolet photoelectron spectroscopy (XPS/UPS) under ultra-high vacuum (UHV). XPS spectra were analysed in order to investigate changes to elemental composition and physical structure. Peak asymmetry in the measured C 1s spectra is found to be a clear indicator of a transition in both physical structure and increased electrical conductivity. The in-situ XPS measurement of pyrolysis is effective in isolating changes in oxygen composition solely due to the pyrolysis process. Oxygen concentration, C 1s peak asymmetry and C 1s peak positions are strong indicators of semiconducting SU-8 transitioning to conducting glass-like carbon. For SU-8 pyrolysed above temperatures of 500 ° C, a clear development is observed in the material structure and composition towards a carbon rich conducting network indicative of glass-like carbon. UPS spectra were analysed to investigate the changes in secondary electron cut-off (SECO) and valence band maximum (VBM) as the SU-8 layer is heated in UHV. The changes in SECO and VBM correlates well with the XPS data and a zero binding energy state is observed at 1000 ° C. • In-situ observation of glass-like carbon formation. • X-ray photoelectron spectroscopy showing transformation of non - conductive SU-8 to a conductive thin film. • Observation of structural oxygen reduction between 300 and 600 °C leading to the formation of a carbon rich network. • Appearance of various features in UPS data in-line with compositional changes observed in XPS data. • Appearance of zero binding energy state at 1000 ° C.

CarbonVol. 245
Aberystwyth University (GB), Cardiff University (GB)
Engineering and Physical Sciences Research Council
Openalex Percentile: Top 85%
Astro and Planetary Science
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