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Title: Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state

Journal Article · · Astrophysics (Engl. Transl.); (United States)
DOI:https://doi.org/10.1007/BF01005831· OSTI ID:5704429

Some periodic regimes have been obtained numerically for the shell of a neutron star in a superstrong magnetic field of strength 10 to the 12th Oe and having density 100,000 g/cm. The periodic regimes are due to anomalies in the equation of state.

Research Organization:
Institut Teoreticheskoi i Prikladnoi Mekhaniki, Novosibirsk, USSR
OSTI ID:
5704429
Journal Information:
Astrophysics (Engl. Transl.); (United States), Vol. 20
Country of Publication:
United States
Language:
English

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Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
NEUTRON STARS
HYDRODYNAMICS
STAR MODELS
DENSITY
EQUATIONS OF STATE
GRAVITATIONAL FIELDS
EQUATIONS
FLUID MECHANICS
MATHEMATICAL MODELS
MECHANICS
PHYSICAL PROPERTIES
STARS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources