589 research outputs found
Electrical conductivity tensor of dense plasma in magnetic fields
Electrical conductivity of finite-temperature plasma in neutron star crusts
is studied for applications in magneto-hydrodynamical description of compact
stars. We solve the Boltzmann kinetic equation in relaxation time approximation
taking into account the anisotropy of transport due to the magnetic field, the
effects of dynamical screening in the scattering matrix element and corre-
lations among the nuclei. We show that conductivity has a minimum at a non-zero
temperature, a low-temperature decrease and a power-law increase with
increasing temperature. Selected numerical results are shown for matter
composed of carbon, iron, and heavier nuclei present in the outer crusts of
neutron star.Comment: 12 pages, 5 figures, supplemental material contains 21 tables.
Proceedings of "The Modern Physics of Compact Stars and Relativistic Gravity
2015", 30 September 2015 - 3 October 2015 Yerevan, Armeni
Electrical Resistivity and Hall Effect in Binary Neutron-Star Mergers
We examine the range of rest-mass densities, temperatures and magnetic fields
involved in simulations of binary neutron-star mergers and identify the
conditions under which the ideal-magnetohydrodynamics approximation breaks down
and hence the magnetic-field decay should be accounted for. We use recent
calculations of the conductivities of warm correlated plasma in envelopes of
compact stars and find that the magnetic-field decay timescales are much larger
than the characteristic timescales of the merger process for lengthscales down
to a meter. Because these are smaller than the currently available resolution
in numerical simulations, the ideal-magnetohydrodynamics approximation is
effectively valid for all realistic simulations. At the same time, we find that
the Hall effect can be important at low densities and low temperatures, where
it can induce a non-dissipative rearrangement of the magnetic field. Finally,
we mark the region in temperature and density where the hydrodynamic
description breaks down.Comment: 10 pages, 4 figures, v2: minor changes, matches published version;
v1: 9 page, 4 figure
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