Neutron Stars Properties and Crust Movements in Post-glitch Epoch

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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Latex, 4 pages, 3 eps figures

Scientific paper

Using a new numerical code with non-uniform adapted mesh, we study the
changes produced in the global properties of neutron stars by the motion of
matter in crust region during post-glitch epoch. Our numerical analysis shows
that these changes may contribute to explain the observed spin-down of
rotational frequency.

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