Abstract

Abstract Molecular dynamics simulations for water and aqueous solutions of apolar rare gases have been carried out in order to study the dependence of hydration structures on solute species. The solute species under investigation were neon and xenon. The structures and thermodynamic properties relevant to the hydration processes were analyzed based upon the quenching of the system to local potential energy minima. It was found that the two solutes give rise to qualitatively different hydration structures; the introduction of Xe atoms make a significant water structure enhancement, increasing the population of pentagonal hydrogen bond network. The solution of neon with usual size parameter and combining rule failed to reproduce the experimentally observed properties. The structural change in quenched state was seen in the Ne solution where a somewhat larger size parameter was adopted. In normal mode analysis, the potential energy was expanded up to quadratic order around quenched configurations. Free energ...

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.