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- W3021507645 abstract "At present there exist several well-grounded models of pulsar radiation which do not exactly coincide with each other [ e.g. Ruderman and Sutherland (1975), Cheng and Ruderman (1980), Arons and Sharlemann (1979), Arons (1981)]. The creation of a dense, relativistic, electron-positron plasma in the polar regions of rotating neutron star magnetospheres is the point of similarity between these models. Surely the pulsar radiation should be generated in such a plasma. The plasma density near the stellar surface is np ≃ 10 16 e to 10 17 cm –3 , and the average Lorentz-factor of the particles is γ p = 3 to 10. The plasma is penetrated by the beam of “primary” electrons, extracted from the stellar surface and accelerated by the electric field. The beam parameters are as follows: n b = 7 x 10 –2 B 0 P –1 , where P is the pulsar period and B 0 magnetic field at the stellar surface and γ b = 3 x 10 6 to 10 7 ." @default.
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- W3021507645 date "1992-01-01" @default.
- W3021507645 modified "2023-09-26" @default.
- W3021507645 title "On a Possible Mechanism of Pulsar Radiation" @default.
- W3021507645 doi "https://doi.org/10.1017/s0002731600155222" @default.
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