<正> Considering the density dependence of quark mass,we investigate the phase transition between the(un-paired)strange quark matter and the color-flavor-locked matter,which are supposed to be two candidates for...<正> Considering the density dependence of quark mass,we investigate the phase transition between the(un-paired)strange quark matter and the color-flavor-locked matter,which are supposed to be two candidates for the groundstate of strongly interacting matter.We find that if the current mass of strange quark m_s is small,the strange quarkmatter remains stable unless the baryon density is very high.If m_s is large,the phase transition from the strangequark matter to the color-flavor-locked matter in particular to its gapless phase is found to be different from the resultspredicted by previous works.A complicated phase diagram of three-flavor quark matter is presented,in which thecolor-flavor-locked phase region is suppressed for moderate densities.展开更多
Considering the effect of one-gluon-exchange interaction between quarks,the color-flavor locked strange quark matter and strange stars are investigated in a new quark mass density-dependent model.It is found that the ...Considering the effect of one-gluon-exchange interaction between quarks,the color-flavor locked strange quark matter and strange stars are investigated in a new quark mass density-dependent model.It is found that the color-flavor locked strange quark matter can be more stable if the one-gluon-exchange effect is included.The lower density behavior of the sound velocity in this model is different from the previous results.Moreover,the new equation of state leads to a heavier acceptable maximum mass,supporting the recent observation of a compact star mass as large as about 2 times the solar mass.展开更多
基金The project supported by National Natural Science Foundation of China under Grant No. 10405012
文摘<正> Considering the density dependence of quark mass,we investigate the phase transition between the(un-paired)strange quark matter and the color-flavor-locked matter,which are supposed to be two candidates for the groundstate of strongly interacting matter.We find that if the current mass of strange quark m_s is small,the strange quarkmatter remains stable unless the baryon density is very high.If m_s is large,the phase transition from the strangequark matter to the color-flavor-locked matter in particular to its gapless phase is found to be different from the resultspredicted by previous works.A complicated phase diagram of three-flavor quark matter is presented,in which thecolor-flavor-locked phase region is suppressed for moderate densities.
基金partially supported by Scientific Research Foundation for the Returned Overseas Chinese Scholars,State Education Ministry(SRF for ROCS,SEM)the National Natural Science Foundation of China(NSFC)under Contract(10875058)
基金support from the National Natural Science Foundation of China (Grant Nos.11135011 and 11045006)the Key Project of Chinese Academy of Sciences (No.Y12A0A0012)
文摘Considering the effect of one-gluon-exchange interaction between quarks,the color-flavor locked strange quark matter and strange stars are investigated in a new quark mass density-dependent model.It is found that the color-flavor locked strange quark matter can be more stable if the one-gluon-exchange effect is included.The lower density behavior of the sound velocity in this model is different from the previous results.Moreover,the new equation of state leads to a heavier acceptable maximum mass,supporting the recent observation of a compact star mass as large as about 2 times the solar mass.