The millisecond pulsar and neutron star structure

DOI10.1007/BF00650153zbMath0582.76049WikidataQ68606679 ScholiaQ68606679MaRDI QIDQ1068629

Armen V. Sarkissian

Publication date: 1985

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

pulsarsurface magnetic fieldbimetric theory of gravitationideal neutron gaslimit of rotational stabilityneutron star modelsreal baryon gasRotational stability conditionslow down rate of pulsar modelsstate of cold superdense matter

Mathematics Subject Classification ID

Gas dynamics (general theory) (76N15) Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Slowly rotating superdense configurations in Rosen's bimetric theory of gravitation
• Plasma at densities above the nuclear
• A bi-metric theory of gravitation
• Unnamed Item

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