Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state
Abstract
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.
- Authors:
- Publication Date:
- Research Org.:
- Institut Teoreticheskoi i Prikladnoi Mekhaniki, Novosibirsk, USSR
- OSTI Identifier:
- 5704429
- Resource Type:
- Journal Article
- Journal Name:
- Astrophysics (Engl. Transl.); (United States)
- Additional Journal Information:
- Journal Volume: 20
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 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
Citation Formats
Mukanova, B G. Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state. United States: N. p., 1984.
Web. doi:10.1007/BF01005831.
Mukanova, B G. Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state. United States. https://doi.org/10.1007/BF01005831
Mukanova, B G. 1984.
"Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state". United States. https://doi.org/10.1007/BF01005831.
@article{osti_5704429,
title = {Numerical simulation of gas-dynamic processes in shells of neutron stars with allowance for anomalies in the equation of state},
author = {Mukanova, B G},
abstractNote = {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.},
doi = {10.1007/BF01005831},
url = {https://www.osti.gov/biblio/5704429},
journal = {Astrophysics (Engl. Transl.); (United States)},
number = ,
volume = 20,
place = {United States},
year = {Sat Sep 01 00:00:00 EDT 1984},
month = {Sat Sep 01 00:00:00 EDT 1984}
}
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