Abstract
We present binding energies of hydrogen states in magnetic fields B = 0 to B ≈ 5 × 108 T, relevant for the modeling of the atmospheres of magnetic white dwarfs and neutron stars. We analyzed states with magnetic quantum number m = 0, ..., –4 and included states up to a principal quantum number n = 15 for a total of 300 states. Due to a sophisticated data point selection we can interpolate any energy value for each of these states with an absolute precision of at least 10–6 Ry for any magnetic field strength. Further, and also as a function of the magnetic field strength, we present dipole strengths of all transitions between these states relevant for the Lyman, Balmer, Paschen, and Brackett series, with similarly high precision.
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