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© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.

Abstract

MXenes are a family of two-dimensional nanomaterials. Titanium carbide MXene (Ti3C2Tx-MXene), reported in 2011, is the first inorganic compound reported among the MXene family. In the present work, we report on the study of the composition and various physical properties of Ti3C2Tx-MXene nanomaterial, as well as their temperature evolution, to consider MXenes for space applications. X-ray diffraction, thermal analysis and mass spectroscopy measurements confirmed the structure and terminating groups of the MXene surface, revealing a predominant single OH layer character. The temperature dependence of the specific heat shows a Debye-like character in the measured range of 2 K–300 K with a linear part below 10 K, characteristic of conduction electrons of metallic materials. The electron density of states (DOS) calculations for Ti3C2OH-MXene reveal a significant DOS value at the Fermi level, with a large slope, confirming its metallic character, which is consistent with the experimental findings. The temperature dependence of electrical resistivity of the MXene samples was tested for a wide temperature range (3 K–350 K) and shows a decrease on lowering temperature with an upturn at low temperatures, where negative magnetoresistance is observed. The magnetoresistance versus field is approximately linear and increases its magnitude with decreasing temperature. The magnetization curves are straight lines with temperature-independent positive slopes, indicating Pauli paramagnetism due to conduction electrons.

Details

Title
Temperature Evolution of Composition, Thermal, Electrical and Magnetic Properties of Ti3C2Tx-MXene
Author
Srivatsa, Shreyas 1   VIAFID ORCID Logo  ; Tokarz, Waldemar 2 ; Przewoźnik, Janusz 2   VIAFID ORCID Logo  ; Strączek, Tomasz 3   VIAFID ORCID Logo  ; Grabowski, Krzysztof 4   VIAFID ORCID Logo  ; Rutkowski, Paweł 5   VIAFID ORCID Logo  ; Uhl, Tadeusz 4   VIAFID ORCID Logo  ; Kulawik, Jan 6 ; Kata, Dariusz 5 ; Madej, Dominika 5   VIAFID ORCID Logo  ; Lis, Jerzy 5 ; Kapusta, Czesław 2 

 Space Technology Centre, AGH University of Krakow, 30-059 Krakow, Poland; [email protected] (S.S.); [email protected] (K.G.); [email protected] (T.U.) 
 Faculty of Physics and Applied Computer Science, AGH University of Krakow, 30-059 Krakow, Poland; [email protected] (J.P.); [email protected] (C.K.) 
 National Synchrotron Radiation Centre SOLARIS, Jagiellonian University, Czerwone Maki 98, 30-392 Kraków, Poland; [email protected] 
 Space Technology Centre, AGH University of Krakow, 30-059 Krakow, Poland; [email protected] (S.S.); [email protected] (K.G.); [email protected] (T.U.); Department of Robotics and Mechatronics, AGH University of Krakow, 30-059 Krakow, Poland 
 Faculty of Materials Science and Ceramics, AGH University of Krakow, al. A. Mickiewicza 30, 30-059 Krakow, Poland; [email protected] (P.R.); [email protected] (D.K.); [email protected] (D.M.); [email protected] (J.L.) 
 Kraków Division, Łukasiewicz Research Network—Institute of Microelectronics and Photonics, 30-701 Kraków, Poland; [email protected] 
First page
2199
Publication year
2024
Publication date
2024
Publisher
MDPI AG
e-ISSN
19961944
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
3059605744
Copyright
© 2024 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.