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- W3119274314 abstract "We study the impact of strong magnetic fields on the pasta phases that are expected to exist in the inner crust of neutron stars. We employ the relativistic mean field model to describe the nucleon interaction and use the self-consistent Thomas-Fermi approximation to calculate the nonuniform matter in neutron star crust. The properties of pasta phases and crust-core transition are examined. It is found that as the magnetic field strength $B$ is less than ${10}^{17}$ G, the effects of magnetic field are not evident comparing with the results without magnetic field. As $B$ is stronger than ${10}^{18}$ G, the onset densities of pasta phases and crust-core transition density decrease significantly, and the density distributions of nucleons and electrons are also changed obviously." @default.
- W3119274314 created "2021-01-18" @default.
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- W3119274314 date "2021-01-11" @default.
- W3119274314 modified "2023-10-15" @default.
- W3119274314 title "Impact of strong magnetic fields on the inner crust of neutron stars" @default.
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- W3119274314 doi "https://doi.org/10.1103/physrevc.103.015804" @default.
- W3119274314 hasPublicationYear "2021" @default.
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