Palapanidis, K., Stergioulas, N. and Lander, S. K. (2015) Magnetized neutron stars with superconducting cores: Effect of entrainment. Monthly Notices of the Royal Astronomical Society, 452 (3). pp. 3246-3255. ISSN 0035-8711
Full text not available from this repository.Abstract
We construct equilibrium configurations of magnetized, two-fluid neutron stars using an iterative numerical method.Working in Newtonian framework we assume that the neutron star has two regions: the core, which is modelled as a two-component fluid consisting of type-II superconducting protons and superfluid neutrons, and the crust, a region composed of normal matter. Taking a new step towards more complete equilibrium models, we include the effect of entrainment, which implies that a magnetic force acts on neutrons, too.We consider purely poloidal field cases and present improvements to an earlier numerical scheme for solving equilibrium equations, by introducing new convergence criteria. We find that entrainment results in qualitative differences in the structure of field lines along the magnetic axis.
Item Type: | Article |
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Uncontrolled Keywords: | methods: numerical,stars: neutron,astronomy and astrophysics,space and planetary science ,/dk/atira/pure/subjectarea/asjc/3100/3103 |
Faculty \ School: | Faculty of Science > School of Mathematics (former - to 2024) |
UEA Research Groups: | Faculty of Science > Research Groups > Quantum Matter Faculty of Science > Research Groups > Numerical Simulation, Statistics & Data Science |
Related URLs: | |
Depositing User: | LivePure Connector |
Date Deposited: | 28 Jan 2020 03:52 |
Last Modified: | 07 Nov 2024 12:42 |
URI: | https://ueaeprints.uea.ac.uk/id/eprint/73803 |
DOI: | 10.1093/mnras/stv1536 |
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