Mathematics – Probability
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.1002b&link_type=abstract
American Astronomical Society, 181st AAS Meeting, #10.02; Bulletin of the American Astronomical Society, Vol. 24, p.1133
Mathematics
Probability
Scientific paper
The ionization equilibrium in highly magnetized (B=10(10) to 10(12) G) hydrogen is investigated at temperatures from 5 eV to 50 keV and densities in the range 10(-3) to 10(3) g/cm(3) . We have used the occupation probability formalism in order to take into account the pressure and density effects. The occupation probabilities used are slightly modified as compared to those derived by Hummer and Mihalas. We find that pressure ionization degree varies with the form of microfield distribution function. The non-ionized fraction is increased by the magnetic field in most of the parameter space. It is large enough so that the bound-free absorption must be taken into account in realistic models of neutron star atmospheres.
Bulik Tomasz
Pavlov George G.
Potekhin A.
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