Inhomogeneous superconductors and inhomogeneous superfluids appear in a
variety of contexts including quark matter at extreme densities, fermionic
systems of cold atoms, type-II cuprates, and organic superconductors. In the
present review the focus is on properties of quark matter at high baryonic
density, which may exist in the interior of compact stars. The conditions
realized in these stellar objects tend to disfavor standard symmetric BCS
pairing and may favor an inhomogeneous color superconducting phase. The
properties of inhomogeneous color superconductors are discussed in detail and
in particular of crystalline color superconductors. The possible astrophysical
signatures associated with the presence of crystalline color superconducting
phases within the core of compact stars are also reviewed.Comment: Added 3 figures, added section II F, added section with conclusions.
Several references added. Improved the quality of the presentation and
removed various typos. Almost matches the version accepted for publication of
Reviews of Modern Physic