Book contents
- Frontmatter
- Contents
- Group photograph
- List of participants
- Preface
- Reviews
- 1 Equations of state in stellar structure and evolution
- 2 Equation of state of stellar plasmas
- 3 Statistical mechanics of quantum plasmas. Path integral formalism
- 4 Onsager-molecule approach to screening potentials in strongly coupled plasmas
- 5 Astrophysical consequences of the screening of nuclear reactions
- 6 Crystallization of dense binary ionic mixtures. Application to white dwarf cooling theory
- 7 Non crystallized regions of White dwarfs. Thermodynamics. Opacity. Turbulent convection
- 8 White dwarf crystallization
- 9 Gravitational collapse versus thermonuclear explosion of degenerate stellar cores
- 10 Neutron star crusts with magnetic fields
- 11 High pressure experiments for astrophysics
- 12 Equation of state of dense hydrogen and the plasma phase transition; A microscopic calculational model for complex fluids
- 13 The equation of state of fluid hydrogen at high density
- 14 A comparative study of hydrogen equations of state
- 15 Strongly coupled ionic mixtures and the H/He equation of state
- 16 White dwarf seismology: Influence of the constitutive physics on the period spectra
- 17 Helioseismology: the Sun as a strongly-constrained, weakly-coupled plasma
- 18 Transport processes in dense stellar plasmas
- 19 Cataclysmic variables: structure and evolution
- 20 Giant planet, brown dwarf, and low-mass star interiors
- 21 Searches for brown dwarfs
- 22 Jovian seismology
- Observational projects
- Posters
4 - Onsager-molecule approach to screening potentials in strongly coupled plasmas
from Reviews
Published online by Cambridge University Press: 07 September 2010
- Frontmatter
- Contents
- Group photograph
- List of participants
- Preface
- Reviews
- 1 Equations of state in stellar structure and evolution
- 2 Equation of state of stellar plasmas
- 3 Statistical mechanics of quantum plasmas. Path integral formalism
- 4 Onsager-molecule approach to screening potentials in strongly coupled plasmas
- 5 Astrophysical consequences of the screening of nuclear reactions
- 6 Crystallization of dense binary ionic mixtures. Application to white dwarf cooling theory
- 7 Non crystallized regions of White dwarfs. Thermodynamics. Opacity. Turbulent convection
- 8 White dwarf crystallization
- 9 Gravitational collapse versus thermonuclear explosion of degenerate stellar cores
- 10 Neutron star crusts with magnetic fields
- 11 High pressure experiments for astrophysics
- 12 Equation of state of dense hydrogen and the plasma phase transition; A microscopic calculational model for complex fluids
- 13 The equation of state of fluid hydrogen at high density
- 14 A comparative study of hydrogen equations of state
- 15 Strongly coupled ionic mixtures and the H/He equation of state
- 16 White dwarf seismology: Influence of the constitutive physics on the period spectra
- 17 Helioseismology: the Sun as a strongly-constrained, weakly-coupled plasma
- 18 Transport processes in dense stellar plasmas
- 19 Cataclysmic variables: structure and evolution
- 20 Giant planet, brown dwarf, and low-mass star interiors
- 21 Searches for brown dwarfs
- 22 Jovian seismology
- Observational projects
- Posters
Summary
Abstract
The solution of the exact integral equation for the liquid pair-structure in the asymptotic strong coupling limit for the plasma, as mapped on the Onsager charge-smearing optimization for the energy lower bound, features “Onsager atoms” and “Onsager molecules”. The universal properties of this asymptotic limit make it a natural reference starting point for an asymptotic strong coupling expansion for the fluid structure and thermodynamics, playing the role of an “ideal liquid” state. In particular, the leading strong coupling terms for the potential energy, direct correlation functions, and screening potentials for the Coulomb and Yukawa mixtures (corresponding to classical plasmas and electron screened classical plasmas), with full thermodynamic consistency, are presented. These are in complete agreement with the Alastuey-Jancovici analysis of early simulations data by Hansen in strong coupling, and with recent highly accurate simulations data of Ogata, Iyetomi, and Ichimaru. Data analysis errors lead Ogata, Iyetomi, and Ichimaru to incorrect results for the short range screening potentials in strong coupling. Their calculations for the short range screening potentials, bridge functions, and enhancement factors for nuclear reaction rates in strongly coupled plasmas, should be revised.
La solution de l'équation intégrate exacte pour la structure du liquide dans la limite asymptotique de couplage fort pour le plasma, calquée sur l'optimisation de charge d'Onsager pour la limite inférieure de l'énergie, met en évidence des “atomes d'Onsager” et des “molécules d'Onsager”.
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- Chapter
- Information
- The Equation of State in AstrophysicsIAU Colloquium 147, pp. 78 - 105Publisher: Cambridge University PressPrint publication year: 1994
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