Virial Equation of State for a Granular System
arXiv:2402.17100 · doi:10.1140/epje/s10189-024-00412-z
Abstract
The equation of state for an ideal gas is simple, which is . In the case of imperfect gases where mutual interactions among the constituents are important, pressure can be expressed as the series expansion of density with appropriate coefficients, known as virial coefficients . In this paper, we have obtained the first four virial coefficients for a model interaction potential using multidimensional Monte-Carlo integration and importance sampling methods. Next, we perform molecular dynamics simulations with the same for a many-particle system to obtain as a function of and . We compare our numerical data with the virial equation of state.
15 Pages, 7 Figures
References in corpus (9)
- Cluster Formation and The Virial Equation of State of Low-Density Nuclear Matter
- Ninth and Tenth Order Virial Coefficients for Hard Spheres in D Dimensions
- A Second Relativistic Mean Field and Virial Equation of State for Astrophysical Simulations
- Analytic calculation of B4 for hard spheres in even dimensions
- Equation of State of nuclear matter in a Virial expansion of nucleons and nuclei
- The fourth virial coefficient of a fluid of hard spheres in odd dimensions
- Clustering and Velocity Distributions in Granular Gases Cooling by Solid Friction
- Granular Fluids with Solid Friction and Heating
- Intruder Dynamics in a Frictional Granular Fluid: A Molecular Dynamics Study