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[en] After a brief review of the phenomena expected in cold dense quark matter, colour superconductivity and colour-flavour locking, we sketch some implications of recent developments in our understanding of cold dense quark matter for the physics of compact stars. We give a more detailed summary of our recent work on crystalline colour superconductivity and the consequent realization that (some) pulsar glitches may originate in quark matter. (author)
Journal
Journal of Physics. G, Nuclear and Particle Physics; ISSN 0954-3899; 
; v. 27(3); p. 541-555
; v. 27(3); p. 541-555