Abstract
This paper outlines the problems of the quasi-steady matter-antimatter boundary layers discussed in Klein-Alfvén's cosmological theory, and a crude model of the corresponding ambiplasma balance is presented:
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(i)
At interstellar particle densities, no well-defined boundary layer can exist in presence of neutral gas, nor can such a layer be sustained in an unmagnetized fully ionized ambiplasma.
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(ii)
Within the limits of applicability of the present model, sharply defined boundary layers are under certain conditions found to exist in a magnetized ambiplasma. Thus, at beta values less than unity, a steep pressure drop of the low-energy components of matter and antimatter can be balanced by a magnetic field and the electric currents in the ambiplasma.
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(iii)
The boundary layer thickness is of the order of 2x 0≃10/BT 1/40 metres, whereB is the magnetic field strength in MKS units andT 0 the characteristic temperature of the low-energy components in the layer.
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Lehnert, B. Problems of matter-antimatter boundary layers. Astrophys Space Sci 46, 61–71 (1977). https://doi.org/10.1007/BF00643754
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DOI: https://doi.org/10.1007/BF00643754