Neutron Stars Properties and Crust Movements in Post-glitch Epoch
classification
🌀 gr-qc
keywords
changescrustepochneutronnumericalpost-glitchpropertiesstars
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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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