Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection

Details Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...498..667z&link_type=abstract

Astronomy and Astrophysics, Volume 498, Issue 3, 2009, pp.667-670

Astronomy and Astrophysics

Astrophysics

2

Radiation Mechanisms: Non-Thermal, Galaxies: Active, Ism: Cosmic Rays

Scientific paper

Context: In powerful cosmic nonthermal radiation sources with a dominant magnetic field self generation, partition between the energy densities in magnetic fields and relativistic electrons is expected. As the electrons cool by synchrotron emission, the magnetic field strength becomes time-dependent and adjusts itself to the actual kinetic energy density of the radiating electrons. Aims: For the case of instantaneous injection of power law distributed electrons with a flat power law spectral index, the nonlinear synchrotron fluence is calculated. Results: For flat (spectral index 1

Affiliated with

Also associated with

No associations

Rating

Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection 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 Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1105509