Calculation of equation of state in stellar interiors becomes difficult as contained gas deviates from perfect gas. We present a method for the calculation of electron pressure in terms of density and temperature in the presence of degeneracy. The method is applicable for T < 10(9) K, and requires complete ionization
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
publisherln this paper, next subject is discussed, §32. The equation of state of an ideal gas. Here ...
A knowledge of the equation of state (EOS) of matter is necessary to describe the dependence of its ...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
The formalism of Glassgold, Heckrotte, and Watson for the expansion of the quantum-mechanical grand ...
We give a complete review of various expansions which may be used for quick and accurate computing o...
Tables of the electron pressure and kinetic energy for a partially degenerate, relativistic, ideal e...
$^{1}$ R. Latter, Phys. Rev. 99, 1854 (1955).Author Institution: General Dynamics/General Atomic Div...
Stellar modelling challenges the physicist to provide accurate data for a lot of processes in a wide...
Recent advances in computational condensed matter theory have yielded accurate calculations of prope...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
Considering the Helmholtz free energy which provides detailed knowledge of the charged many-particle...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
The equations of state (EoS) and other thermodynamic properties of plasmas of the light elements H, ...
Entanglement distance is the maximal separation between two entangled electrons in a degenerate elec...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
publisherln this paper, next subject is discussed, §32. The equation of state of an ideal gas. Here ...
A knowledge of the equation of state (EOS) of matter is necessary to describe the dependence of its ...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
The formalism of Glassgold, Heckrotte, and Watson for the expansion of the quantum-mechanical grand ...
We give a complete review of various expansions which may be used for quick and accurate computing o...
Tables of the electron pressure and kinetic energy for a partially degenerate, relativistic, ideal e...
$^{1}$ R. Latter, Phys. Rev. 99, 1854 (1955).Author Institution: General Dynamics/General Atomic Div...
Stellar modelling challenges the physicist to provide accurate data for a lot of processes in a wide...
Recent advances in computational condensed matter theory have yielded accurate calculations of prope...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
Considering the Helmholtz free energy which provides detailed knowledge of the charged many-particle...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
The equations of state (EoS) and other thermodynamic properties of plasmas of the light elements H, ...
Entanglement distance is the maximal separation between two entangled electrons in a degenerate elec...
The Fermi-Thomas model has been used to derive the equation of state of matter at high pressures and...
publisherln this paper, next subject is discussed, §32. The equation of state of an ideal gas. Here ...
A knowledge of the equation of state (EOS) of matter is necessary to describe the dependence of its ...
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