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Title: In-medium chiral condensate beyond linear density approximation

Journal Article · · Physical Review. C, Nuclear Physics
; ;  [1]
  1. Physik Department, Technische Universitaet Muenchen, D-85747 Garching (Germany)

In-medium chiral perturbation theory is used to calculate the density dependence of the quark condensate <qq>. The corrections beyond the linear density approximation are obtained by differentiating the interaction contributions to the energy per particle of isospin-symmetric nuclear matter with respect to the pion mass. Our calculation treats systematically the effects from one-pion exchange (with m{sub {pi}}-dependent vertex corrections), iterated 1{pi}-exchange, and irreducible 2{pi}-exchange including intermediate {delta}(1232)-isobar excitations, with Pauli-blocking corrections up to three-loop order. We find a strong and nonlinear dependence of the ''dropping'' in-medium condensate on the actual value of the pion (or light quark) mass. In the chiral limit, m{sub {pi}}=0, chiral restoration appears to be reached already at about 1.5 times normal nuclear matter density. By contrast, for the physical pion mass, m{sub {pi}}=135 MeV, the in-medium condensate stabilizes at about 60% of its vacuum value above that same density. Effects from 2{pi}-exchange with virtual {delta}(1232)-isobar excitations turn out to be crucial in generating such pronounced deviations from the linear density approximation above {rho}{sub 0}. The hindered tendency toward chiral symmetry restoration provides a justification for using pions and nucleons as effective low-energy degrees of freedom at least up to twice nuclear matter density.

OSTI ID:
21068152
Journal Information:
Physical Review. C, Nuclear Physics, Vol. 77, Issue 2; Other Information: DOI: 10.1103/PhysRevC.77.025204; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2813
Country of Publication:
United States
Language:
English

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