It appears you don't have support to open PDFs in this web browser. To view this file, Open with your PDF reader
Abstract
Earth-abundant antimony trisulfide (Sb2S3), or simply antimonite, is a promising material for capturing natural energies like solar power and heat flux. The layered structure, held up by weak van-der Waals forces, induces anisotropic behaviors in carrier transportation and thermal expansion. Here, we used stress as mechanical stimuli to destabilize the layered structure and observed the structural phase transition to a three-dimensional (3D) structure. We combined in situ x-ray diffraction (XRD), Raman spectroscopy, ultraviolet-visible spectroscopy, and first-principles calculations to study the evolution of structure and bandgap width up to 20.1 GPa. The optical band gap energy of Sb2S3 followed a two-step hierarchical sequence at approximately 4 and 11 GPa. We also revealed that the first step of change is mainly caused by the redistribution of band states near the conduction band maximum. The second transition is controlled by an isostructural phase transition, with collapsed layers and the formation of a higher coordinated bulky structure. The band gap reduced from 1.73 eV at ambient to 0.68 eV at 15 GPa, making it a promising thermoelectric material under high pressure.
Antimonite (Sb2S3) has potential applications for solar energy, but how its layered structure changes under pressure is incompletely understood. Here diamond anvil cell experiments supported by first principles calculations offer a structural explanation for experimentally observed phase transitions.
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details


1 Center for High Pressure Science and Technology Advanced Research, Shanghai, P.R. China (GRID:grid.410733.2); Central South University, Key Laboratory of Metallogenic Prediction of Nonferrous Metals and Geological Environment Monitor, Ministry of Education, Changsha, P.R. China (GRID:grid.216417.7) (ISNI:0000 0001 0379 7164)
2 Center for High Pressure Science and Technology Advanced Research, Shanghai, P.R. China (GRID:grid.410733.2)
3 University of Hawai’i at Manoa, Hawai’i Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, Honolulu, USA (GRID:grid.410445.0) (ISNI:0000 0001 2188 0957)
4 Central South University, Key Laboratory of Metallogenic Prediction of Nonferrous Metals and Geological Environment Monitor, Ministry of Education, Changsha, P.R. China (GRID:grid.216417.7) (ISNI:0000 0001 0379 7164)
5 Center for High Pressure Science and Technology Advanced Research, Shanghai, P.R. China (GRID:grid.410733.2); Chinese Academy of Sciences, CAS Center for Excellence in Deep Earth Science, Guangzhou Institute of Geochemistry, Guangzhou, P.R. China (GRID:grid.9227.e) (ISNI:0000000119573309)