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Superconducting K strings in high density QCD
Author(s) -
Kirk B. W. Buckley,
Ariel Zhitnitsky
Publication year - 2002
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2002/08/013
Subject(s) - physics , quantum chromodynamics , string (physics) , superconductivity , strange matter , neutron star , symmetry (geometry) , condensation , particle physics , quark , field (mathematics) , theoretical physics , condensed matter physics , quantum mechanics , geometry , mathematics , pure mathematics , thermodynamics
Recently it has been argued that the ground state of high density QCD islikely be a combination of the CFL-phase along with condensation of the K^0field. This state spontaneously breaks a global U(1)_Y symmetry, therefore onewould expect the formation of U(1)_Y global strings. We discuss the corestructure of these strings and demonstrate that under some conditions theglobal U(1)_Y symmetry may not be restored inside the string, in contrast withthe standard expectations. Instead, K^+ condensation occurs inside the core ofthe string if a relevant parameter \cos\theta_K = \mkzero^2/\mu_eff^2 is largerthan some critical value \theta_K > \theta_crit. If this phenomenon happens,the U(1)_Y strings become superconducting and may considerably influence themagnetic properties of dense quark matter, in particular in neutron stars.Comment: 10 pages, 2 Postscript figures. Discussion improved and acknowledgement adde

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