Quantitative Broadband Optical Spectroscopy of Freestanding Ti 3 C 2 T x MXene Films: Unveiling Intrinsic Bulk Charge Carrier Dynamics
Source abstract
Abstract
Micrometer-thick freestanding MXene films offer a rare opportunity to probe intrinsic bulk optical and electronic properties without the influence of a substrate. Yet, quantitative optical constants over a broadband spectral range remain elusive due to the mechanically flexible nature of such films. Here, we report the first comprehensive far-infrared-to-ultraviolet (150–36,000 cm –1 ) optical spectroscopic study of freestanding Ti 3 C 2 T x MXene films with thicknesses of 1 and 4 μm. By a combination of attaching the freestanding films on flat and smooth brass plates and using an in situ metal-evaporation method, we obtained highly reliable reflectance spectra. Kramers–Kronig analysis, coupled with a two-Drude-Lorentz model, reveals multiple free-carrier populations at the Fermi level, yielding carrier densities of 7.31 × 10 21 and 7.50 × 10 21 cm –3 and mobilities of 8.15 and 4.98 cm 2 V –1 s –1 for the 1- and 4-μm-thick freestanding films, respectively. The spectra further identify a 1.61 eV feature arising from interband-plasmon coupling and a 3.84 eV interband transition, with small thickness dependence, highlighting the bulk-dominated plasmonic response in micrometer-scale films. This work establishes a quantitative, noncontact framework for mapping intrinsic charge dynamics in MXenes, unlocking pathways for their integration into broadband plasmonic, optoelectronic, infrared, and THz devices.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: MXene and MAX Phase Materials · 2D Materials and Applications · Heusler alloys: electronic and magnetic properties
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics
Sungkyunkwan University
School of Advanced Materials Science and Engineering
Swiss Federal Laboratories for Materials Science and Technology, Empa
School of Chemical Engineering
Department of Physics and Astronomy
McMaster University
Funding
National Research Foundation of Korea · Ministry of Science, ICT, and Future Planning, Republic of Korea
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