Chiral-symmetry restoration in clustered hadronic matter

  • G. KreinEmail author


Chiral-symmetry restoration is usually discussed in the context of quark matter, a system of deconfined quarks. However, many systems like stable nuclei and neutron stars have quarks confined within nucleons. In the present paper we use a Fermi sea of three-quark clusters instead of a Fermi sea of deconfined quarks to investigate the in-medium quark condensate. We find that an enhancement of the chiral breaking in clustered matter as claimed in the literature is not a consequence of the clustering but rather dependent on the microscopic model dynamics.


Neutron Star Quark Matter Microscopic Model Quark Condensate Hadronic Matter 
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© Springer-Verlag Berlin/Heidelberg 2003

Authors and Affiliations

  1. 1.Instituto de Física TeóricaUniversidade Estadual PaulistaSão PauloSP, Brazil

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