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The dense core of compact stars is the natural medium for the realization of color superconductivity. A common characteristic of such astrophysical objects is their strong magnetic fields, especially those of the so called magnetars. In…

High Energy Physics - Phenomenology · Physics 2010-01-23 Efrain J. Ferrer

It is quite plausible that color superconductivity occurs in the inner regions of neutron stars. At the same time, it is known that strong magnetic fields exist in the interior of these compact objects. In this paper we discuss some…

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

We find that the chromomagnetic instability existing in neutral two- flavor color superconductivity at moderate densities is removed by the formation of an inhomogeneous condensate of charged gluons and the corresponding induction of a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Efrain J. Ferrer , Vivian de la Incera

We discuss the Meissner effect for a color superconductor formed by cold dense quark matter. Though color and ordinary electromagnetism are broken in a color superconductor, there is a linear combination of the photon and a gluon that…

High Energy Physics - Phenomenology · Physics 2010-02-04 M. Alford , J. Berges , K. Rajagopal

In this paper the neutral 2SC phase of color superconductivity is investigated in the presence of a magnetic field and for diquark coupling constants and baryonic densities that are expected to characterize neutron stars. Specifically, the…

High Energy Physics - Phenomenology · Physics 2024-12-23 Shuai Yuan , Bo Feng , Efrain J. Ferrer , Alejandro Pinero

In this talk I review some of the main findings on magnetism in color superconductivity. The physical characteristic of the different phases that are reached by increasing the applied magnetic field in a three-flavor color superconductor at…

Nuclear Theory · Physics 2011-10-11 Efrain J. Ferrer

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 2010-07-29 Brian Niebergal , Rachid Ouyed , Rodrigo Negreiros , Fridolin Weber

In this talk I will discuss how the in-medium magnetic field can influence the gluon dynamics in a three-flavor color superconductor. It will be shown how at field strengths comparable to the charged gluon Meissner mass a new phase can be…

Nuclear Theory · Physics 2011-09-28 Efrain J. Ferrer

We investigate the effects of an external magnetic field in the gluon dynamics of a color superconductor with three massless quark flavors. In the framework of gluon mean-field theory at asymptotic densities, we show that the long-range…

High Energy Physics - Phenomenology · Physics 2009-11-11 Efrain J. Ferrer , Vivian de la Incera

In this paper I discuss the magnetic phases of the three-flavor color superconductor. These phases can take place at different field strengths in a highly dense quark system. Given that the best natural candidates for the realization of…

Nuclear Theory · Physics 2008-11-26 Vivian de la Incera

Neutron stars may harbour the true ground state of matter in the form of strange quark matter. If present, this type of matter is expected to be a color superconductor, a consequence of quark pairing with respect to the color/flavor degrees…

Solar and Stellar Astrophysics · Physics 2015-06-04 K. Glampedakis , D. I. Jones , L. Samuelsson

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

Extremely strong magnetic fields of the order of $10^{15}\,{\rm G}$ are required to explain the properties of magnetars, the most magnetic neutron stars. Such a strong magnetic field is expected to play an important role for the dynamics of…

High Energy Astrophysical Phenomena · Physics 2017-10-25 Jerome Guilet , Ewald Mueller , Hans-Thomas Janka , Tomasz Rembiasz , Martin Obergaulinger , Pablo Cerda-Duran , Miguel-Angel Aloy

The behaviour of the magnetic field of a neutron star with a superconducting quark matter core is investigated in the framework of the Ginzburg-Landau theory. We take into account the simultaneous coupling of the diquark condensate field to…

High Energy Physics - Phenomenology · Physics 2014-11-17 D. M. Sedrakian , D. Blaschke

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 show a possibility that strong ``magnetic field'' $\sim 10^{15} $G is produced by color ferromagnetic quark matter in neutron stars. In the quark matter a color magnetic field is generated spontaneously owing to Savvidy mechanism and a…

High Energy Physics - Phenomenology · Physics 2013-05-29 Aiichi Iwazaki

We give an introduction crystalline color superconductivity, arguing that it is likely to occur wherever quark matter in which color-flavor locking does not occur is found. We survey the properties of this form of quark matter, and argue…

High Energy Physics - Phenomenology · Physics 2009-11-07 Krishna Rajagopal

After a brief review of the phenomena expected in cold dense quark matter, color superconductivity and color-flavor locking, we sketch some implications of recent developments in our understanding of cold dense quark matter for the physics…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mark Alford , Jeffrey A. Bowers , Krishna Rajagopal

Compact stars serve as natural systems where matter exists at densities far beyond those achievable in laboratory experiments. Among them, magnetars are expected to possess interior magnetic fields that may reach values of the order of…

High Energy Astrophysical Phenomena · Physics 2026-05-01 Monika Sinha , Vivek Baruah Thapa

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
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