5–10 Jul 2021
Europe/Rome timezone

Calculation of the tensor components of the kinetic coefficients of arbitrarily degenerate electrons in the neutron star crust.

9 Jul 2021, 07:10
20m
Talk in the parallel session MHD processes near compact objects MHD Processes Near Compact Objects

Speaker

Maria Glushikhina (Space Research Institute (IKI RAN))

Description

Analytical expressions are obtained for four tensors of kinetic coefficients from the solution of the Boltzmann equation by the Chapman-Enskog method in the 3-polynomial approximation, taking into account electron-electron collisions for the case of nondegenerate electrons in a magnetic field.
For strongly degenerate electrons, asymptotically accurate analytical expressions for the thermal conductivity tensor, thermo-diffusion, diffusion, and diffusion thermal effect in the Lorentz approximation are obtained for the first time, taking into account the magnetic field. This solution has a much more complex dependence on the magnetic field than the dependencies in previous publications.
For the special case of partial degeneracy at $\epsilon_{f}/kT = 1.011$, analytical expressions for the kinetic coefficients in the absence of a magnetic field are obtained from the solution of the Boltzmann equation in the 3-polynomial approximation. It is shown that the convergence of the polynomial approximation to the exact value is slower than for non-degenerate electrons.

Primary authors

Prof. Gennady Bisnovatyi-Kogan (Space Research Institute (IKI RAN)) Maria Glushikhina (Space Research Institute (IKI RAN))

Presentation materials

There are no materials yet.

Proceedings

Paper