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

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

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011raa....11..679x&link_type=abstract

Research in Astronomy and Astrophysics, Volume 11, Issue 6, pp. 679-686 (2011).

Astronomy and Astrophysics

Astrophysics

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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