z-logo
open-access-imgOpen Access
Microscopic structure of water at elevated pressures and temperatures
Author(s) -
Christoph J. Sahle,
Christian Sternemann,
Christian Schmidt,
Susi Lehtola,
Sandro Jahn,
Laura Simonelli,
Simo Huotari,
Mikko Hakala,
Tuomas Pylkkänen,
Alexander Nyrow,
Kolja Mende,
Metin Tolan,
K. Hämäläinen,
Max Wilke
Publication year - 2013
Publication title -
proceedings of the national academy of sciences
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 5.011
H-Index - 771
eISSN - 1091-6490
pISSN - 0027-8424
DOI - 10.1073/pnas.1220301110
Subject(s) - supercritical fluid , raman spectroscopy , molecular dynamics , hydrogen bond , chemistry , molecule , density functional theory , atmospheric temperature range , chemical physics , spectral line , thermodynamics , ab initio , materials science , computational chemistry , physics , organic chemistry , optics , astronomy
We report on the microscopic structure of water at sub- and supercritical conditions studied using X-ray Raman spectroscopy, ab initio molecular dynamics simulations, and density functional theory. Systematic changes in the X-ray Raman spectra with increasing pressure and temperature are observed. Throughout the studied thermodynamic range, the experimental spectra can be interpreted with a structural model obtained from the molecular dynamics simulations. A spatial statistical analysis using Ripley’s K-function shows that this model is homogeneous on the nanometer length scale. According to the simulations, distortions of the hydrogen-bond network increase dramatically when temperature and pressure increase to the supercritical regime. In particular, the average number of hydrogen bonds per molecule decreases to ≈0.6 at 600 °C andp = 134 MPa.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom