Crystalline color superconductors

被引：145

作者：

Anglani, Roberto ^{[1
]}

Casalbuoni, Roberto ^{[2
,3
]}

Ciminale, Marco ^{[4
]}

Ippolito, Nicola ^{[5
]}

Gatto, Raoul ^{[6
]}

Mannarelli, Massimo ^{[7
]}

Ruggieri, Marco ^{[8
]}

机构：

[1] CNR ISSIA, Natl Res Council, Inst Intelligent Syst Automat, I-70126 Bari, Italy

[2] Univ Florence, Dept Phys, I-50019 Sesto Fiorentino, Fl, Italy

[3] INFN, I-50019 Sesto Fiorentino, Fl, Italy

[4] MIUR, I-00153 Rome, Italy

[5] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[6] Univ Geneva, Dept Phys Theor, CH-1211 Geneva, Switzerland

[7] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67100 Laquila, Italy

[8] Univ Catania, Dept Phys & Astron, I-95125 Catania, Italy

来源：

REVIEWS OF MODERN PHYSICS | 2014年 / 86卷 / 02期

关键词：

EQUATION-OF-STATE; EFFECTIVE-FIELD THEORY; FINITE BARYON DENSITY; NEUTRON-STAR; QUARK MATTER; SYMMETRY-BREAKING; FLAVOR LOCKING; 3RD FAMILY; LOFF PHASE; INTERNAL TEMPERATURE;

D O I：

10.1103/RevModPhys.86.509

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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.

引用

页码：509 / 561

页数：53

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