Co-crystal structure of HCN:ethane
SND-ID: 2024-529. Version: 1. DOI: https://doi.org/10.71870/5xrf-na15
Associated documentation
Download all files
Citation
Creator/Principal investigator(s)
Martin Rahm
- Chalmers University of Technology, Department of Chemistry and Chemical Engineering
Fernando Izquierdo-Ruiz
- Chalmers University of Technology, Department of Chemistry and Chemical Engineering
Research principal
Description
Data for PBE-D3(BJ)/DZVP molecular dynamics simulation of 1:4 intercalated co-crystal structure (readable e.g., by VMD). Simulation made using CP2K, v2024.1 span 20ps.
Movie of molecular dynamics simulation of 1:4 intercalated co-crystal structure at 90 K (mp4 file)
Data contains personal data
No
Language
Contributor(s)
Fernando Izquierdo-Ruiz
- Chalmers University of Technology
Hilda Sandström
- Chalmers University of Technology
Fernando Izquierdo-Ruiz
- Chalmers University of Technology
Hilda Sandström
- Chalmers University of Technology
Alvaro Lobato
- Chalmers University of Technology
Martin Rahm
- Chalmers University of Technology
Commissioning organisation
Chalmers University of Technology
Research area
Theoretical chemistry (Standard för svensk indelning av forskningsämnen 2011)
Keywords
Dft, Astrokemi, Co-crystals, Titan, Kristallstrukturprediktion, Molekyldynamik
Izquierdo-Ruiz F, Cable M, Hodyss R, Vu T, Sandström H, Lobato A, et al. Polar Opposites Attract on Saturn’s Moon Titan. ChemRxiv. 2024; doi:10.26434/chemrxiv-2024-t8l8v This content is a preprint and has not been peer-reviewed.
DOI:
https://doi.org/10.26434/chemrxiv-2024-t8l8v