A possible decrease in the equilibrium radius of a neutron star due to the effect of a superstrong magnetic field
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Publication:1762254
DOI10.1007/s11182-012-9785-6zbMath1259.85005OpenAlexW2081610283MaRDI QIDQ1762254
Publication date: 23 November 2012
Published in: Russian Physics Journal (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s11182-012-9785-6
Quantum field theory on curved space or space-time backgrounds (81T20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Special relativity (83A05) Galactic and stellar structure (85A15) Electromagnetic theory (general) (78A25) Galactic and stellar dynamics (85A05)
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