The Influence of Electron Impact Ionization in the Relativistic Pickup of Interstellar Neutrals

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4

Elementary Particles, Galaxies: Active, Galaxies: Jets, Plasmas, Radiation Mechanisms: Nonthermal

Scientific paper

The influence of interstellar neutrals on the relativistic pickup process in jets of active galactic nuclei is investigated. It is assumed that the jet plasma consists of thermally distributed electron-positron pairs. Using the formalism of Weaver and the electron impact ionization cross section of Lotz for neutral hydrogen H I and neutral helium He I, the corresponding ionization lengths in the comoving outflow frame of reference are calculated. For nonrelativistic pair temperatures the ionization lengths are constants and of order ~=2×1014Γ/np,8 cm, where Γ denotes the outflow bulk Lorentz factor and np,8 is the comoving pair density in units of 108 cm-3. We estimate that about 5%-9% of the neutrals are ionized in the outflow region. After ionization these pickup ions and electrons form an anisotropic backward-propagating beam distribution in the outflow plasma, which initiates two-stream instabilities.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Influence of Electron Impact Ionization in the Relativistic Pickup of Interstellar Neutrals does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Influence of Electron Impact Ionization in the Relativistic Pickup of Interstellar Neutrals, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Influence of Electron Impact Ionization in the Relativistic Pickup of Interstellar Neutrals will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-913461

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.