Wigner solution of the quark gap equation
Wigner solution of the quark gap equation
复制标题
夸克间隙方程的维格纳解
DOI:
10.1140/epjc/s10052-018-6264-4
复制
发表时间:
2018
影响因子:
4.4
通讯作者:
Zong Hong-Shi
中科院分区:
文献类型:
--
作者:
Cui Zhu-Fang;Xu Shu-Sheng;Li Bo-Lin;Sun An;Zhang Jing-Bo;Zong Hong-Shi
Solutions and their evolutions of the quark gap equation are studied within the Nambu–Jona–Lasinio model, which is a basic issue for studying the QCD phase structure and locating the possible critical end point. It is shown that in the chiral limit case of the vacuum, chiral symmetry will hold if the coupling strengthGis small, then the system only has the Wigner solution at. If increasingG, two symmetric minima will appear as the positive and “negative” Nambu solutions, however, the solutionnow corresponds to a maximum instead of a minimum of the thermodynamical potential, so is not a physically stable state anymore (we call it “pseudo-Wigner solution”). Besides, it is shown that as the current quark massmincreases, the pseudo-Wigner solution will become negative, and disappear together with the negative Nambu solution ifmis large enough. Similar things happen if we increase the temperature or quark chemical potential. Some interesting phenomenon is, from somea second local minimum will show up. Asincreases gradually, it will be stabler than the Nambu solution, survives even the Nambu solution disappears, and approachesm, which are just the features of the Wigner solution we expect.