Abstract

This study is performed with the aim of gaining insights into the possible applicability of the quark-hadron continuity concept, not only in the idealized case of three-flavor symmetric quark matter, but also for the transition from neutron matter to two-flavor quark matter. A key issue is the continuity between neutron superfluidity and a corresponding superfluid quark phase produced by $d$-quark pairing. Symmetry arguments are developed and relevant dynamical mechanisms are analyzed. It is pointed out that the $^3P_2$ superfluidity in dense neutron matter has a direct analogue in the $^3P_2$ pairing of $d$-quarks in two-flavor quark matter. This observation supports the idea that the quark-hadron continuity hypothesis may be valid for such systems. Possible implications for neutron stars are briefly discussed.

Highlights

  • This study is performed with the aim of gaining insights into the possible applicability of the quarkhadron continuity concept, in the idealized case of three-flavor symmetric quark matter, and for the transition from neutron matter to two-flavor quark matter

  • Two decades ago a conceptual framework for a continuous connection between hadronic and quark phases of dense matter described by quantum chromodynamics (QCD) was suggested in Ref. [1], based on the exact matching of symmetry breaking patterns and low-lying excitations in both domains

  • It is important to note that Uð1ÞB corresponding to baryon number conservation is spontaneously broken, so that the color-flavor locked (CFL) state can be regarded as a superfluid

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Summary

INTRODUCTION

Two decades ago a conceptual framework for a continuous connection between hadronic and quark phases of dense matter described by quantum chromodynamics (QCD) was suggested in Ref. [1], based on the exact matching of symmetry breaking patterns and low-lying excitations in both domains. A Ginzburg-Landau analysis shows that matter at sufficiently low temperature goes through a smooth crossover from the hadronic to the quark phase as one increases the baryon density [3]. Such a continuous crossover is realized in a three-flavor Nambu–Jona-Lasinio (NJL) model [4]. Neutron pairing in the 3P2 state starts to develop and becomes the dominant pairing mechanism for nB > n0, inward bound towards the neutron star core region This realization of 3P2 superfluidity is based on the observed pattern of nucleon-nucleon (NN) scattering phase shifts [25,26].

ABUNDANCE OF NEUTRONS AND DOWN QUARKS IN NEUTRON STAR MATTER
SYMMETRY ARGUMENTS FOR QUARK-HADRON CONTINUITY
Three-flavor case
Two-flavor case
REARRANGEMENT OF THE ORDER-PARAMETER OPERATORS
Three-flavor symmetric case
Two-flavor 1S0 superfluid matter
Two-flavor 3P2 superfluid matter
DYNAMICAL PROPERTIES FAVORING TRIPLET P-WAVE PAIRING
OLSGE ðrÞ
SUPPORTING ARGUMENTS
Coupling to the energy-momentum tensor
Aspects of neutron star cooling phenomenology
SUMMARY AND CONCLUSIONS
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