Mémoire Online: Les étoiles à neutrons (Etude des propriétés cinétiques)

Mémoire Online les étoiles à neutrons (Etude des propriétés cinétiques), tutoriel & guide de travaux pratiques en pdf.

Introduction
Chapter I: Neutron star an overview
I-1 Introduction
I-2 History of neutron star physics
I-3 Basic parameters of neutron star
I-4 Structure of neutron star envelopes
I-5 Magnetic field and its evolution
Chapter II: General properties of neutron star’s Coulomb plasma
II-1 The method of minimizing the free energy
II-2 Parameters of the plasma
II-2-1 General settings
II-2-2 Electrons
II-2-3 Ions
II-3 Fully ionized Coulomb plasma
II-3-1 Ideal electron gas
II-3-2 Coulomb crystal (harmonic approximation)
II-3-3 Ionic Coulomb liquid (theory)
II-3-4 Structural factor: Multiphonon processes
II-3-3 Ionic Coulomb liquid (theory)
II-3-4 Structural factor: Multiphonon processes
II-3-4-a The structure factor of the classical isotropic plasma
II-3-4-b Structure factor of the Coulomb crystal and Debye-Waller factor
II-3-4-c Multiphonon processes
II-3-5 Melting
II-3-6 Polarization of the electrons in the Coulomb liquid
II-3-7 Polarization of the electrons in the Coulomb crystal
Chapter III: Electronic transport coefficients without magnetic field
A Basic relations for the electronic transport coefficients
III-1 Boltzmann equation: General relationships
III-2 Electron-electron scattering
III-3 Electron-ion scattering. Approximation of the relaxation time
III-4 General expressions for the nondegenerate plasma
III-5 Strongly degenerate electron gas
III-6 Matthiessen’s rule
B Outline OCP calculations (IOFFE model)
III-7 Scattering of electrons on ions
III-8 Overall approximation for the outer shells
Chapter IV: Electrical and thermal conductivities in dense plasma
A Theoretical contribution
IV-1 The effect of the nuclear form factor
IV-1-1 The Gaussian Charge distribution
IV-1-2 The homogeneous sphere Charge distribution
IV-1-3 The exponential charge distribution
IV-2 Multi components plasma
IV-3 Scattering of strongly degenerate Electron by electrons
B Simulation
1- Nuclear form factor effects
2- Multi components plasma
3- Scattering of strongly degenerate Electron by electrons
Chapter V: Viscosity coefficients and thermal and magnetic effects
A Theoretical contribution:
V-1 Viscosity
V-1-1 On the theory of viscosity
V-1-2 Determination of the correctives terms
V-2 Thermal and magnetic effects on kinetic coefficients
V-2-1 Problema One: “ magnetic fields”:
V-2-2 Problema Two: “ partially degenerate electrons”
V-2-3 Interpolation formula
B Simulation
Conclusion
……….

les étoiles à neutrons

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