Quarkyonic matter (QyM) is a large Nc phase of cold dense quark matter recently suggested by McLerran and Pisarski [1]. The main feature of QyM is the existence of asymptotically free quarks deep in the Fermi sea and confined excitations at the Fermi surface. The quarks lying deep in the Fermi sea are weakly interacting because they are hard to be excited due to Pauli blocking. Their interactions are hence very energetic and the confining part of the interaction does not play any role [2]. On the other hand, excitations of quarks within a shell of width ΛQCD from the Fermi surface interact through infrared singular gluons at large Nc and hence are confined. In has been recently argued [3, 4] that chiral symmetry can be broken in QyM through the formation of a translational non-invariant condensate that arises from the pairing between a quark with momentum p, and the hole formed by removing a quark with opposite momentum p from the Fermi surface. The inhomogeneous condensate that forms in QyM is a linear combination of the chiral condensate 〈ψψ〉, and a spin-one, isosinglet odd-parity condensate of 〈ψσψ〉. Here z is the direction of motion of the wave. At each given patch of the Fermi surface, z is the direction perpendicular to the surface. The authors of Ref. [3] called this combination of two inhomogeneous condensates a Quarkyonic Chiral Spiral (QyCS). The 〈ψσψ〉 component corresponds to the condensation of an electric dipole moment. The QyCS is then characterized by a spatial oscillation between chiral and electric dipole condensates that breaks parity and gives rise to an inhomogeneous electric field. On the other hand, a common feature of heavy-ion collisions is the generation of strong magnetic fields that are produced in peripheral collisions by the positively charged ions moving at almost the speed of light. For the Au-Au collisions at the Relativistic Heavy Ion Collider (RHIC) at BNL the field produced is estimated to be ∼ 10G [5]. Even though this magnetic field decays quickly, it only decays to a tenth of the original value for a time scale of order of the inverse of the saturation scale at RHIC [5], hence it may influence the properties of the QCD phases probed by the experiment. Strong magnetic fields will likely be also generated in future experiments planned at the Facility for Antiproton and Ion Research (FAIR) at GSI, the Nuclotron-Ion Collider Facility (NICA) at JINR, and the Japan Proton Accelerator Research Complex (JPARK) at JAERI, all of which intend to complement the experiments at RHIC by reaching regions of even higher densities and intermediate to low temperatures in the QCD phase map. In this paper we discuss the effects of an external magnetic field on QyM. As will be seen below, the presence of a magnetic field of strength comparable to the square of the QCD scale gives rise to the formation of a second chiral spiral, given by a spatial oscillation between a pion condensate 〈ψγ5ψ〉 and a spin-one condensate 〈ψγγψ〉. The spin-one condensate corresponds to an inhomogeneous magnetic moment in the direction of the field.
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