Cold quark matter in astrophysics of compact stars
Armen SedrakianInstitute for Theoretical Physics, J. W. Goethe‐University, D‐60438 Frankfurt am Main, GermanyLeonardo AngeliniPietro ColangeloFulvia De FazioG. E. BrunoDonato CreanzaE. Nappi
2010en
ABI
Annotatsiya
The appearance of quark matter in the centers of compact stars has a number of astrophysical implications. In this contribution I discuss the structure and stability of compact stars, gravitational radiation from non‐axisymmetric deformations, and nucleation and dynamics of vortices (flux tubes) in the color superconducting phases.
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