Role of the pressure anisotropy in the relativistic pulsar wind

DOI10.1007/BF01008390zbMath0516.76106MaRDI QIDQ1052918

D. Beaufils, E. Asseo

Publication date: 1983

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

neutron staranisotropic pressurehot relativistic MHD wind analysisinfinite electric conductivityLichnerowicz magnetic vectornon-scalar pressurepulsar windradiative lossestransverse particle momentum

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05)

Related Items (1)

On the theory of translationally invariant magnetohydrodynamic equilibria with anisotropic pressure and magnetic shear

Cites Work

• The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisions

This page was built for publication: Role of the pressure anisotropy in the relativistic pulsar wind