First-order phase transitions in rotating hybrid stars and pulsar glitches

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The first order deconfinement phase transitions in rotating hybrid stars
are studied and it is found that if the surface tension is sufficiently
large, the transition from metastable hadron matter to stable mixed
hadron-quark matter during the spin-down history of a hybrid star can
cause a glitch.

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