Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..205h&link_type=abstract
In ESA Plasma Astrophys. p 205-208 (SEE N85-22270 12-90)
Astronomy and Astrophysics
Astrophysics
2
Electron-Positron Pairs, Electron-Positron Plasmas, High Temperature Plasmas, Pair Production, Relativistic Plasmas, Annihilation Reactions, Electron Density (Concentration), Magnetic Field Configurations, Magnetic Flux
Scientific paper
Steady states of thermal electron-positron pair plasmas at mildly relativistic temperatures and in strong magnetic fields are investigated. The pair density in steady-state equilibrium where pair production balances annihilation is found as a function of temperature, magnetic field strength and source size, by means of a numerical calculation which includes pair production attenuation and Compton scattering of the photons. It is found that there is a maximum pair density for each value of temperature and field strength, and also a source size above which optically thin equilibrium states do not exist.
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