Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..201s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 201-204.
Astronomy and Astrophysics
Astrophysics
Cosmic Plasma, Electron-Positron Plasmas, Hadrons, Nonuniform Plasmas, Plasma Cooling, Relativistic Plasmas, Electron Scattering, Plasma Resonance, Positrons, Time Response
Scientific paper
The time scale for cooling of a relativistic Maxwellian electron-positron plasma by production of hadronic resonances (ρ, ω, φ, Ψ, Ψarcmin) in energetic e+ - e- collisions is calculated. The comparison with electromagnetic cooling processes, in particular elastic two-body collisions, shows that the hadronic time scale is at least two orders of magnitude larger than the two-body relaxation time scale in plasmas without magnetic field.
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