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Related papers: Crystalline Color Superconductivity

200 papers

We discuss gapless color superconductivity for neutral quark matter in beta equilibrium at zero as well as at nonzero temperature. Basic properties of gapless superconductors are reviewed. The current progress and the remaining problems in…

Nuclear Theory · Physics 2007-05-23 Igor A. Shovkovy , Stefan B. Ruester , Dirk H. Rischke

Superconducting state is achieved through quantum condensation of Cooper pairs which are new types of charge carriers other than single electrons in normal metals. The theory established by Bardeen-Cooper-Schrieffer (BCS) in 1957 can…

Superconductivity · Physics 2025-02-20 Hai-Hu Wen

Surface effects in strange-quark matter play an important role for certain observables which have been proposed in order to identify strange stars, and color superconductivity can strongly modify these effects. We study the surface of color…

Nuclear Theory · Physics 2009-09-29 Micaela Oertel , Michael Urban

The best natural candidates for the realization of color superconductivity are quark stars -not yet confirmed by observation- and the extremely dense cores of compact stars, many of which have very large magnetic fields. To reliably predict…

Nuclear Theory · Physics 2008-11-26 Efrain J. Ferrer , Vivian de la Incera

We study effects of two-flavor color superconductivity on the structure of strange dwarfs, which are stellar objects with similar masses and radii with ordinary white dwarfs but stabilized by the strange quark matter core. We find that…

Astrophysics · Physics 2009-06-23 Masayuki Matsuzaki , Etsuchika Kobayashi

We provide analytical and numerical evidence that the attractive two-dimensional Kitaev model on a lattice with mirror symmetry demonstrates unusual 'intrinsic' phase at half filling. This phase emerges in the phase diagram at the boundary…

Superconductivity · Physics 2020-01-08 Adam Lowe , Miguel Ortuno , Igor V Yurkevich

The core region of a neutron star may feature quark matter in the color-flavor- locked (CFL) phase. The CFL condensate breaks the baryon number symmetry, such that the phenomenon of superfluidity arises. If the core of the star is rotating,…

Nuclear Theory · Physics 2016-12-21 Mark G. Alford , S. Kumar Mallavarapu , Tanmay Vachaspati , Andreas Windisch

Compact stars made of quark matter rather than confined hadronic matter, are expected to form a color superconductor. This superconductor ought to be threaded with rotational vortex lines, within which the star's interior magnetic field is…

High Energy Astrophysical Phenomena · Physics 2010-04-06 Brian Niebergal , Rachid Ouyed , Rodrigo Negreiros , Fridolin Weber

The equation of state of deconfined strongly interacting matter at high densities remains an open question, with effects from quark pairing in the preferred color-flavor-locked (CFL) ground state possibly playing an important role. Recent…

High Energy Physics - Phenomenology · Physics 2025-11-21 Andreas Geißel , Tyler Gorda , Jens Braun

Because of a logarithmic enhancement from soft, collinear magnetic gluons, in dense quark matter the gap for a color superconducting condensate with spin zero depends upon the QCD coupling constant g not as exp(-1/g^2), like in BCS theory,…

Nuclear Theory · Physics 2009-12-30 R. D. Pisarski , D. H. Rischke

The phase diagram of strongly interacting matter is explored as a function of temperature and baryon number density. We investigate the possible simultaneous formation of condensates in the conventional quark--anti-quark channel (breaking…

High Energy Physics - Phenomenology · Physics 2010-02-04 J. Berges

Magnetic properties of quark matter and its relation to the microscopic origin of the magnetic field observed in compact stars are studied. Spontaneous spin polarization appears in high-density region due to the Fock exchange term, which…

High Energy Physics - Phenomenology · Physics 2007-05-23 T. Tatsumi , E. Nakano , K. Nawa

We investigate neutral quark matter with homogeneous and inhomogeneous color condensates at finite temperature in the frame of an extended NJL model. By calculating the Meissner masses squared and gap susceptibility, the uniform color…

High Energy Physics - Phenomenology · Physics 2010-05-07 Lianyi He , Meng Jin , Pengfei Zhuang

We study a model for color superconductivity with both three colors and massless flavors including quark pairing. By using the Hamiltonian in the color-flavor basis we can calculate the quantum entropy. From this we are able to further…

High Energy Physics - Phenomenology · Physics 2007-05-23 D. E. Miller , A. Tawfik

Random matrix theory (RMT) provides a powerful framework for analyzing universal features of strongly coupled physical systems. In quantum chromodynamics (QCD), cold quark matter at asymptotically high density is expected to exhibit color…

High Energy Physics - Theory · Physics 2026-05-19 Takuya Kanazawa

QCD predicts matter at high density should exhibit color superconductivity. We review briefly several pertinent properties of color superconductivity and then discuss how baryons are realized in color superconductors. Especially, we explain…

High Energy Physics - Phenomenology · Physics 2009-03-16 Deog Ki Hong

Deconfined quark matter at asymptotically high densities is weakly coupled, due to the asymptotic freedom of Quantum Chromodynamics. In this weak-coupling regime, bulk thermodynamic properties of quark matter, assuming a trivial ground…

High Energy Physics - Phenomenology · Physics 2024-07-25 Andreas Geißel , Tyler Gorda , Jens Braun

We show a possibility that there exists a color ferromagnetic state in quark matter, in which a color magnetic field is spontaneously generated. The state arises between the hadronic state and the color superconducting state when the…

Nuclear Theory · Physics 2009-11-10 Aiichi Iwazaki , Osamu Morimatsu

The quantum condensate of Cooper-pairs forming a superconductor was originally conceived to be translationally invariant. In theory, however, pairs can exist with finite momentum $Q$ and thereby generate states with spatially modulating…

We show that within a recently developed nonlocal chiral quark model the critical density for a phase transition to color superconducting quark matter under neutron star conditions can be low enough for these phases to occur in compact star…

Astrophysics · Physics 2009-11-10 Hovik Grigorian , David Blaschke , Dmitri Voskresensky