22–26 Jun 2025
Goerlitz & HZDR Dresden
Europe/Berlin timezone

Transport in ultra-dense plasmas in neutron stars and white dwarfs in magnetic fields

26 Jun 2025, 09:00
40m

Speaker

Armen Sedrakian (Frankfurt Institute for Advanced Studies and University of Wroclaw)

Description

I will review recent work on electrical and thermal conductivity and the electrical and thermal Hall effect in electron-ion plasmas relevant to hot neutron stars, white dwarfs, and binary neutron star mergers, focusing on densities found in the outer crusts of neutron stars and the interiors of white dwarfs. We consider plasma consisting of a single species of ions, which could be either iron $^{56}$Fe or carbon $^{12}$C nuclei. The temperature range explored is from the melting temperature of the solid $T\sim 10^{9}-10^{11}$ K. This covers both degenerate and non-degenerate electron regimes. The impact of magnetic fields on electrical and thermal conductivity is analyzed, showing anisotropy in low-density regions and the presence of the electrical and thermal Hall effect. The transition from a degenerate to non-degenerate regime is characterized by a minimum ratio of conductivities.

Primary author

Armen Sedrakian (Frankfurt Institute for Advanced Studies and University of Wroclaw)

Co-authors

Dr Arus Harutyunyan (Byurakan Astrophysical Observatory, NAS of Armenia) Dr Mekhak Hayrapetyan (Byurakan Astrophysical Observatory, NAS Armenia) Ms Narine Gevorgyan (Byurakan Astrophysical Observatory, NAS of Armenia)

Presentation materials