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Thermal Cyclotron and Annihilation Radiation in Strong Magnetic Fields

Published online by Cambridge University Press:  12 April 2016

V.G. Bezchastnov  and
A.D. Kaminker
V.G. Bezchastnov
Affiliation:
Ioffe Institute of Physics and Technology, 194021, St.Petersburg, Russia
A.D. Kaminker
Affiliation:
Ioffe Institute of Physics and Technology, 194021, St.Petersburg, Russia

Abstract

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The cyclotron and the one-photon annihilation emissions are investigated for a strongly magnetized thermal electron-positron plasmas. The annihilation spectral component is significant when the particle number density N exceeds some critical value, Ncr(T,B). For T ~ 108 − 109 K and B ~ 1012 − 1013 G, this condition can be fulfilled at N < 1022 cm−3, which is realistic for neutron star magnetospheres.

Type
Posters
Information
International Astronomical Union Colloquium , Volume 147: The Equation of State in Astrophysics , 1994 , pp. 550 - 554
Copyright
Copyright © Cambridge University Press 1994

References

Bezchastnov, V.G. and Pavlov, G.G., Astivphys.Sp.Sci. 178, 1, (1991)Google Scholar
Golenetskii, S.V. et al., Nature 307, 41, (1984)CrossRefGoogle Scholar
Harding, A., Astrophys.J. 300, 167, (1986)CrossRefGoogle Scholar
Harding, A., Phys.Reports 206, 327, (1991)CrossRefGoogle Scholar
Mazets, E.P. et al., Astrophys.Sp.Sci. 84, 173, (1982)CrossRefGoogle Scholar