Neutron star spin evolution: A semi-analytical approach

Physics – Condensed Matter

Scientific paper

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Neutron Stars, Pulsars, Magnetic And Electric Fields, Polarization Of Starlight

Scientific paper

We report on a semi-analytical model for studying the evolution of the spin period P of a magnetic neutron star as a function of the baryonic mass load Macc. We have taken into account different equations of state and included rotational deformation effects. The presence of a strong gravitational field has also been considered in the context of general relativity. A comparison with numerical fully relativistic codes shows that our description is accurate within 5%. .

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