Properties of matter in ultrahigh magnetic fields and the structure of the surface of neutron stars
作者： Mikhail A Liberman , B Johansson
DOI: 10.1070/PU1995V038N02ABEH000067
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摘要: The physical properties of atoms, molecules, and solids in ultrahigh magnetic fields B 109 G that are believed to exist on the surface neutron stars discussed. In these fields, atoms strongly deformed elongated along field lines; binding energy ionizing substantially increased interatomic interaction is dramatically changed. This modifies matter at which crucial for modelling pulsar magnetosphere. A scenario magnetosphere evolution proposed suggests free emission a young strong later stage. stage due bound chains alternate heavy light accreted star.
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