Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion

Details Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..448u&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Computer Science

Giant Resonances, Cherenkov Radiation, Isotopes, Ionisation, Giant Resonances, Cherenkov Detectors, Sources Of Radioactive Nuclei, Electronic Excitation And Ionization Of Molecules, Intermediate Molecular States

Scientific paper

The basic types of losses of the ultra relativistic electron-positron pulsar plasma in the upper atmosphere of a star-companion are considered. These types include: ionization losses of the medium atoms, their excitation losses, the losses connected with the energies transferred to the particles of plasma, the formation losses of the recoil δ electrons and Cherenkov radiation losses of moving particles, bremsstrahlung losses, the synchrotron radiation losses and the losses, connected with the inverse Compton emission. It is shown that the most rapid component of pulsar plasma can reach the top of convective zone. The range of kinetic energies of the plasma particles that reach the upper boundary of the convection zone will correspond to the range of the gigantic dipole resonance (GDR). The result of interaction of the pulsar plasma and of the upper atmosphere of examined star-companion will be the non-homogeneous heating of the local zones of photosphere and boundary between the photosphere and zone of convection on the different depths.

Affiliated with

Also associated with

No associations

Rating

Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion 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 Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interaction of the Ultra Relativistic Pulsar Plasma with the Upper Atmosphere of the Star-Companion will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862770