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Improved hard sphere radial distribution function in the CRIS equation of state model A u t h o r s : Benjamin J. Cowen & John H. Carpenter Sandia National Laboratories is a multimission laboratory managed and operated by National


  1. Improved hard sphere radial distribution function in the CRIS equation of state model A u t h o r s : Benjamin J. Cowen & John H. Carpenter Sandia National Laboratories is a multimission laboratory managed and operated by National Technology & Engineering Solutions of Sandia, LLC, a wholly owned subsidiary of Honeywell International Inc., for the U.S. Department of Energy’s National Nuclear Security Administration under contract DE-NA0003525. 1

  2. Background 2 ▪ Accurate equation of state (EOS) models for various materials are needed as input into high-level shock physics codes ▪ The EOS is typically defined in terms of the Helmholtz free energy, which is often split into 3 terms: 𝐵 𝜍, 𝑈 = 𝐵 0 𝜍 + 𝐵 𝑗 𝜍, 𝑈 + 𝐵 𝑓 𝜍, 𝑈 Cold Curve Thermal Electronic Thermal Ionic ▪ The cold curve is used as an input into the CRIS model, which can be obtained from theory, experiment, or both ▪ The output of the CRIS model includes the first two terms of the Helmholtz free energy equation: 𝐵 0 𝜍 + 𝐵 𝑗 𝜍, 𝑈 , which can then be added to the thermal electronic term for a full EOS ▪ The CRIS model has previously been used to develop the equation of state for metals (Au, Mo, Al, Ta, Pb, Ti, Cu, W), gases (H, D 2 , N, O, C, CO, CH 4 , Xe, Ar), and other materials (Basalt, Ice, CaCO 3 , SiO 2 )

  3. ҧ ҧ The CRIS Model 3 • Calculates thermodynamic properties by expanding about a hard sphere reference system • First we start with the free energy of the hard sphere reference fluid 𝐵 0 𝑠 𝑁 𝜚 𝑠, 𝜃 𝑕 𝑠, 𝜃 𝑠 −1 𝑒𝑠 • Then we add the first order term: 𝜚 0 = √2𝜌 3 ׬ 𝜏 0 • 𝜚 𝑠, 𝜃 = scaled cold curve, used as the interaction potential • 𝑕 𝑠, 𝜃 = radial distribution function (RDF) • 𝜃 = packing fraction, 𝜏 0 = hard sphere diameter 𝑠 𝑁 𝑕 𝑠, 𝜃 𝑠 −1 𝑒𝑠 • 𝑠 𝑁 = cutoff radius determined by solving the normalization condition: 1 = √2𝜌 3 ׬ 0 • Up to first order, we have: ҧ 𝐵 = 𝐵 0 + 𝑂 𝜚 0 • We can then calculate the hard sphere diameter by minimizing: 𝜖 ҧ 𝐵 = 0 𝜖𝜃 𝑊,𝑈,𝑂 • The 2 nd order corrections are defined as: • Fluctuation correction: 𝜃 ∗ √2𝜌 𝑠 𝑁 𝑒𝑠 ഥ 𝜃 • Δ𝐵 1 = −𝑂𝑙𝑈 𝜃 𝑕 𝑠, ҧ 𝜃 𝑔 𝜃 𝑒 ҧ 𝜃 3𝜃 ׬ 𝑠 ׬ 𝜏 0 𝜃 𝑒(ഥ 𝜃𝑨) • 𝑔 𝜃 = 𝑒ഥ 𝜃 • Soft sphere correction: 2 𝜃 ∗ 𝜏 0 𝑕 𝑠, 𝜃 ∗ 𝑠 2 𝑒𝑠 • Δ𝐵 2 = −𝑂𝑙𝑈2𝜌𝜍 ׬ 0 𝜃 • The Helmholtz free energy of the system is defined as: 𝐵 = 𝐵 0 + 𝑂 𝜚 0 + Δ𝐵 1 + Δ𝐵 2 KERLEY, G. I. (1980). PERTURBATION THEORY AND THE THERMODYNAMIC PROPERTIES OF FLUIDS. II. THE CRIS MODEL. THE JOURNAL OF CHEMICAL PHYSICS , 73 (1), 478-486.

  4. Challenges with the CRIS model 4 𝑙 𝜃 3 1 + σ 𝑙=1 𝐶 𝑙 𝑙 𝑦𝑕 0 (1, 𝜃) 𝑄𝑊 3𝜃 𝜃 𝜃 𝑑 Z= 4 𝑂𝑙𝑈 = 4𝜃𝑕 0 1, 𝜃 + 1 = 1 + 𝜃 𝑑 −𝜃 + σ 𝑙=1 𝑙𝐵 𝑙 𝑕 𝑦, 𝜃 = 𝐷 𝜃 = 𝜃 𝑑 3 1 + 𝐷 𝜃 𝑦 − 1 3 1 − 𝜃 𝜃 𝑑 • 𝑕 𝑦, 𝜃 does not represent the hard sphere RDF well over the range of integration • ΔA 2 integrates x<1, and there is a pole in 𝑕 𝑦, 𝜃 in this regime • The fit to Z is good for 𝜃 < 0.5 , but is slightly inaccurate for 𝜃 > 0.5 ALDER, B. J., & WAINWRIGHT, T. E. (1960). STUDIES IN MOLECULAR DYNAMICS. II. BEHAVIOR OF A SMALL NUMBER OF ELASTIC SPHERES. THE JOURNAL OF CHEMICAL PHYSICS , 33 (5), 1439-1451. KOLAFA, J., LABÍK, S., & MALIJEVSKÝ, A. (2004). ACCURATE EQUATION OF STATE OF THE HARD SPHERE FLUID IN STABLE AND METASTABLE REGIONS. PHYSICAL CHEMISTRY CHEMICAL PHYSICS , 6 (9), 2335-2340.

  5. Improving the RDF 5 𝑘 𝑗,𝑘=5 𝐷 𝑗𝑘 𝑦 − 1 𝑗 𝑕 𝑦, 𝜃 is fit to a 5 th order polynomial for x ∈ [1:x M ]: 𝑕 𝑦, 𝜃 = 𝑕 0 1, 𝜃 σ 𝑗,𝑘=0 𝜃 • 𝜃 𝑑 • Coefficients are fixed due to asymptotic limits: 𝑕 𝑦,𝜃 𝑕 𝑦,𝜃 • 𝐷 00 = 1 and 𝐷 𝑗0 = 0 for 𝑗 > 0 since 𝑕 0 (1,𝜃) = 1 when 𝜃 = 0 and 𝐷 0𝑘 = 0 for 𝑘 > 0 since 𝑕 0 (1,𝜃) = 1 when 𝑦 = 1 9 3 1 • 2 𝜃 𝑑 , 𝐷 21 = 2 𝜃 𝑑 , 𝐷 31 = 2 𝜃 𝑑 , 𝐷 41 = 𝐷 51 = 0 from the density expansion as 𝜃 → 0 𝐷 11 = − • 20 unconstrained parameters remain 𝑙 1−4,10,14 𝑙𝐵 𝑙 1 3𝜃 𝜃 • Z is refit (first 3 coefficients are the same) so that it is consistent with the 𝑕(𝑦, 𝜃) approximation: 𝑕 0 (1, 𝜃) = 𝜃 𝑑 −𝜃 + σ 𝑙=1 4𝜃 𝜃 𝑑

  6. Effects of Changing the RDF 6 Isotherms Vapor Dome • We used the Lennard-Jones (LJ) potential as a test case, since we know the exact potential • At lower densities, the relative effect of the RDF is not as important since the ideal gas term is dominant • The new RDF improves the pressure, and is more accurate in the liquid regime than the old RDF • The new RDF makes the estimate of the critical point worse VERLET, L., & WEIS, J. J. (1972). EQUILIBRIUM THEORY OF SIMPLE LIQUIDS. PHYSICAL REVIEW A , 5 (2), 939. POTOFF, J. J., & PANAGIOTOPOULOS, A. Z. (2000). SURFACE TENSION OF THE THREE-DIMENSIONAL LENNARD-JONES FLUID FROM HISTOGRAM-REWEIGHTING MONTE CARLO SIMULATIONS. THE JOURNAL OF CHEMICAL PHYSICS , 112 (14), 6411-6415. CAILLOL, J. M. (1998). CRITICAL-POINT OF THE LENNARD-JONES FLUID: A FINITE-SIZE SCALING STUDY. THE JOURNAL OF CHEMICAL PHYSICS , 109 (12), 4885-4893.

  7. Summary & Conclusions 7 • The CRIS model has been used for decades at institutions around the world for developing equations of state for various materials • However, the CRIS model inaccurately models the RDF for the hard spheres • We improved the RDF using a 5 th order polynomial function and added 𝑄𝑊 higher order terms to 𝑂𝑙𝑈 to make it consistent • The improved RDF more accurately models the isotherms of the LJ fluid, compared to molecular dynamics • Unfortunately, the critical point of the LJ fluid is more over-estimated with the new RDF • Since the critical point is extremely sensitive to small changes in the free energy, future work may involve fitting the RDF to have the EOS better match the vapor dome, while maintaining accurate isotherms

  8. 8 Any Questions?

  9. Backup Slides

  10. CRIS Δ A 2 Integration 10 2 𝜃 ∗ 𝜏 0 𝑕 𝑠, 𝜃 ∗ 𝑠 2 𝑒𝑠 • Δ𝐵 2 = −𝑂𝑙𝑈2𝜌𝜍 ׬ 0 𝜃

  11. Isotherms of the LJ Fluid 11 𝐵 = 𝐵 0 + 𝑂 𝜚 0 𝐵 = 𝐵 0 + 𝑂 𝜚 0 + Δ𝐵 1 𝐵 = 𝐵 0 + 𝑂 𝜚 0 + Δ𝐵 1 + Δ𝐵 2 VERLET, L., & WEIS, J. J. (1972). EQUILIBRIUM THEORY OF SIMPLE LIQUIDS. PHYSICAL REVIEW A , 5 (2), 939.

  12. Vapor Dome of the LJ Fluid 12 𝐵 = 𝐵 0 + 𝑂 𝜚 0 𝐵 = 𝐵 0 + 𝑂 𝜚 0 + Δ𝐵 1 𝐵 = 𝐵 0 + 𝑂 𝜚 0 + Δ𝐵 1 + Δ𝐵 2 POTOFF, J. J., & PANAGIOTOPOULOS, A. Z. (2000). SURFACE TENSION OF THE THREE-DIMENSIONAL LENNARD-JONES FLUID FROM HISTOGRAM-REWEIGHTING MONTE CARLO SIMULATIONS. THE JOURNAL OF CHEMICAL PHYSICS , 112 (14), 6411-6415. CAILLOL, J. M. (1998). CRITICAL-POINT OF THE LENNARD-JONES FLUID: A FINITE-SIZE SCALING STUDY. THE JOURNAL OF CHEMICAL PHYSICS , 109 (12), 4885-4893.

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