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Title: Bonding and structure in dense multi-component molecular mixtures

Journal Article · · Journal of Chemical Physics
DOI:https://doi.org/10.1063/1.4934626· OSTI ID:1236706
 [1];  [1]; ORCiD logo [2];  [3];  [2];  [1];  [1]
  1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  2. Univ. Rostock, Rostock (Germany)
  3. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)

We have performed finite-temperature density functional theory molecular dynamics simulations on dense methane, ammonia, and water mixtures (CH4:NH3:H2O) for various compositions and temperatures (2000 K ≤ T ≤ 10000 K) that span a set of possible conditions in the interiors of ice-giant exoplanets. The equation-of-state, pair distribution functions, and bond autocorrelation functions (BACF) were used to probe the structure and dynamics of these complex fluids. In particular, an improvement to the choice of the cutoff in the BACF was developed that allowed analysis refinements for density and temperature effects. We note the relative changes in the nature of these systems engendered by variations in the concentration ratios. As a result, a basic tenet emerges from all these comparisons that varying the relative amounts of the three heavy components (C,N,O) can effect considerable changes in the nature of the fluid and may in turn have ramifications for the structure and composition of various planetary layers.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
SFB 652; AC52-06NA25396
OSTI ID:
1236706
Alternate ID(s):
OSTI ID: 1224734
Report Number(s):
LA-UR-15-22061; JCPSA6
Journal Information:
Journal of Chemical Physics, Vol. 143, Issue 16; ISSN 0021-9606
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 14 works
Citation information provided by
Web of Science

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Laser-driven shock compression of “synthetic planetary mixtures” of water, ethanol, and ammonia journal July 2019
Stabilization of ammonia-rich hydrate inside icy planets journal August 2017
Structural determination of neutral Co n clusters ( n   =  4–10,13) through IR–UV two-color vibrational spectroscopy and DFT calculations journal November 2018
Multicomponent mutual diffusion in the warm, dense matter regime journal September 2019
Benchmarking the effective one-component plasma model for warm dense neon and krypton within quantum molecular dynamics simulation journal February 2020
Ab initio calculation of thermodynamic potentials and entropies for superionic water journal February 2016
Quantum molecular dynamics study on the proton exchange, ionic structures, and transport properties of warm dense hydrogen-deuterium mixtures journal June 2018
Planetary Ices and the Linear Mixing Approximation journal October 2017