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

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

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..321m&link_type=abstract

(Astrofizika, vol. 20, Mar.-Apr. 1984, p. 321-326) Astrophysics (ISSN 0571-7132), vol. 20, no. 2, Sept. 1984, p. 173-176. Transl

Statistics

Computation

Computational Astrophysics, Equations Of State, Gas Dynamics, Neutron Stars, Stellar Envelopes, Stellar Models, Density Distribution, Digital Simulation, Gravitational Fields, Stellar Magnetic Fields

Scientific paper

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.

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