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[ascl:2306.042] CONDUCT: Electron transport coefficients of magnetized stellar plasmas

CONDUCT calculates all components of kinetic tensors in fully ionized electron-ion plasmas at arbitrary magnetic field. It employs a thermal averaging with the Fermi distribution function and can be used when electrons are partially degenerate; it provides, along with the electrical and thermal conductivities, also thermopower (thermoelectric coefficient). CONDUCT takes into account collisions of the electrons with ions and (in solid phase) charged impurities as well as quantum effects on ionic motion in the solid phase. The code's outputs are the longitudinal, transverse, and off-diagonal (Hall) components of electrical and thermal conductivity tensors as well as the components of thermoelectric tensor.

Code site:
https://www.ioffe.ru/astro/conduct/condmag.html https://www.ioffe.ru/astro/conduct/
Used in:
https://ui.adsabs.harvard.edu/abs/2021ApJ...923...64D
Described in:
https://ui.adsabs.harvard.edu/abs/2015SSRv..191..239P
Bibcode:
2023ascl.soft06042P

Views: 712

ascl:2306.042
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