Equation of state and opacities for hydrogen atmospheres of strongly magnetized cooling neutron stars
Potekhin, A. Y. · Shibanov, Yu. A. · Ventura, J.
Original · EN
We study partially ionized hydrogen plasma at temperatures T = 10⁵.⁵-10⁶.⁵ K and magnetic fields B = 10¹²-10¹³ G, typical of photospheres of isolated neutron stars. We construct an analytic model of the plasma free energy and derive a generalized Saha equation which is used to obtain the opacities.
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