scholarly journals Spectral functions for D¯ and D¯0* mesons in nuclear matter with partial restoration of chiral symmetry

2017 ◽  
Vol 96 (1) ◽  
Author(s):  
Daiki Suenaga ◽  
Shigehiro Yasui ◽  
Masayasu Harada
2017 ◽  
Vol 912 ◽  
pp. 012009
Author(s):  
J J Cobos-Martínez ◽  
K. Tsushima ◽  
G. Krein ◽  
A. W. Thomas

1992 ◽  
Vol 45 (4) ◽  
pp. 2015-2018 ◽  
Author(s):  
L. S. Celenza ◽  
A. Pantziris ◽  
C. M. Shakin ◽  
Wen Dong Sun

2003 ◽  
Vol 18 (32) ◽  
pp. 2255-2264 ◽  
Author(s):  
O. A. Battistel ◽  
G. Krein

Chiral symmetry breaking at finite baryon density is usually discussed in the context of quark matter, i.e. a system of deconfined quarks. Many systems like stable nuclei and neutron stars however have quarks confined within nucleons. In this paper we construct a Fermi sea of three-quark nucleon clusters and investigate the change of the quark condensate as a function of baryon density. We study the effect of quark clustering on the in-medium quark condensate and compare results with the traditional approach of modeling hadronic matter in terms of a Fermi sea of deconfined quarks.


2002 ◽  
Vol 28 (8) ◽  
pp. 2265-2273 ◽  
Author(s):  
P Wang ◽  
H Guo ◽  
Y B Dong ◽  
Z Y Zhang ◽  
Y W Yu

2015 ◽  
Vol 91 (9) ◽  
Author(s):  
Takumi Iritani ◽  
Guido Cossu ◽  
Shoji Hashimoto

2007 ◽  
Vol 16 (02n03) ◽  
pp. 325-332 ◽  
Author(s):  
EDUARDO LÜTZ ◽  
MOISÉS RAZEIRA ◽  
CÉSAR A. Z. VASCONCELLOS ◽  
BARDO E. J. BODMANN ◽  
FERNANDO PILOTTO

On the basis of a chiral symmetry transformation, we predict an isovector component for the family of light scalar mesons, i.e. partners of the σ-meson. Such a contribution may be necessary to tune the equation of state of nuclear matter in order to comply with severe constraints from a recent analysis of observational macroscopic properties of neutron stars.


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