Book contents
- Frontmatter
- Contents
- Group photograph
- List of participants
- Preface
- Reviews
- Observational projects
- Posters
- 29 Towards a helioseismic calibration of the equation of state in the solar convective envelope
- 30 Thermal cyclotron and annihilation radiation in strong magnetic fields
- 31 Modified adiabatic approximation for a hydrogen atom moving in a magnetic field
- 32 Computations of static white dwarf models: A must for asteroseismological studies
- 33 The Chandrasekhar mass of a gravitating electron crystal
- 34 Coulomb corrections in the nuclear statistical equilibrium regime
- 35 Molecular Opacities: Application to the Giant Planets
- 36 On Radiative Transfer Near the Plasma Frequency at Strong Coupling
- 37 Effects of Superfluidity on Spheroidal Oscillations of Neutron Stars
- 38 Magnetic Field Decay in the Non-superfluid Regions of Neutron Star Cores
- 39 On the equation of state in Jovian seismology
- 40 Analysis of the screening formalisms in solar and stellar conditions
- 41 Theoretical Description of the Coulomb Interaction by Padé-Jacobi Approximants
- 42 New Model Sequences from the White Dwarf Evolution Code
41 - Theoretical Description of the Coulomb Interaction by Padé-Jacobi Approximants
from Posters
Published online by Cambridge University Press: 07 September 2010
- Frontmatter
- Contents
- Group photograph
- List of participants
- Preface
- Reviews
- Observational projects
- Posters
- 29 Towards a helioseismic calibration of the equation of state in the solar convective envelope
- 30 Thermal cyclotron and annihilation radiation in strong magnetic fields
- 31 Modified adiabatic approximation for a hydrogen atom moving in a magnetic field
- 32 Computations of static white dwarf models: A must for asteroseismological studies
- 33 The Chandrasekhar mass of a gravitating electron crystal
- 34 Coulomb corrections in the nuclear statistical equilibrium regime
- 35 Molecular Opacities: Application to the Giant Planets
- 36 On Radiative Transfer Near the Plasma Frequency at Strong Coupling
- 37 Effects of Superfluidity on Spheroidal Oscillations of Neutron Stars
- 38 Magnetic Field Decay in the Non-superfluid Regions of Neutron Star Cores
- 39 On the equation of state in Jovian seismology
- 40 Analysis of the screening formalisms in solar and stellar conditions
- 41 Theoretical Description of the Coulomb Interaction by Padé-Jacobi Approximants
- 42 New Model Sequences from the White Dwarf Evolution Code
Summary
Abstract
Coulomb interactions for the Free Helmholtz energy and the pressure are studied in a partial new formulation which described more exactly the numerical evaluation of many body theories.
Introduction
With regard to the EOS many activities have been developed to yield results which consider different phenomena, for instance pressure dissoziation and ionisation, degeneracy, relativity, Coulomb- and non-Coulombic interactions, pair production and charge mixing in different chemical compositions.
Various theoretical approaches are used in order to include exchange and correlation effects for fully ionized or partially ionized matter (see e.g. Salpeter and Zapolski 1967, Graboske et al. 1969, Hansen 1973, Pokrant 1977, Fontaine et al. 1977, March and Tosi 1984, Perrot and Dharmawardana 1984, Hubbard and Dewitt 1985, Dandrea et al. 1986, van Horn 1987, Kraeft et al. 1986, Ichimaru et al. 1987, Rogers and DeWitt 1987, Däppen et al. 1988, Ichimaru 1990, Eliezer and Ricci 1991, Saumon and Chabrier 1992).
For many applications (e.g. stellar evolution calculations or astroseismology) it is necessary either to have algebraic formulae for the EOS or extensive tables which supply the input, informations at any density and temperature. As a, first step we present an analytical EOS for fully ionized multicomponent plasmas covering a large density-temperature range. The EOS includes non-ideal effects due to exchange-correlation interactions of charged particles at any degeneracy and is applicable to any chemical mixture. Relativistic effects as well as ionic quantum corrections are taken into account.
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- Chapter
- Information
- The Equation of State in AstrophysicsIAU Colloquium 147, pp. 606 - 611Publisher: Cambridge University PressPrint publication year: 1994
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