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Electron-positron pairs in hot plasma of accretion column in bright X-ray pulsars

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Figure

Figure 1. The chemical potential of electrons calculated as a function of temperature for different number densities of protons at fixed magnetic field strength 10 13 G (top panel), and for  dif-ferent magnetic field strength at fixed number density of pro
Figure 4. The pressure of electron-positron gas along magnetic field lines calculated as a function of temperature for (a) different number densities of protons: 10 25 (black solid line), 10 27 (brown dashed lile) and 10 29 cm −3 (red dashed-dotted line),
Figure 5. The mean molecular weight as a function of temper- temper-ature for different number densities of protons: 10 25 (black solid line), 10 27 (brown dashed lile) and 10 29 cm −3 (red dashed-dotted line) at magnetic field strength fixed at 10 13 G.

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