Abstract

It follows from the analysis of the precision numerical calculations of the energy spectrum of a hydrogen atom in a static magnetic field that the Zeldovich effect (rearrangement of the atomic spectrum) in the spectrum of atomic levels is observed at superstrong magnetic fields B≥5×1011 G. Magnetic fields of such strengths are reached in neutron stars and magnetic white dwarfs. We established a lower bound Bmin for the fields required for this effect to occur.

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