We investigated the properties of strange quark matter in an external strong magnetic field with both confinement and leading-order perturbative interactions considered. It was found that the leading-order perturbative interaction can stiffen the equation of state of magnetized quark matter, while the magnetic field lowers theminimumenergy per baryon. By solving the Tolman-Oppenheimer-Volkoff equations, we obtain the internal structure of strange stars. The maximum mass of strange stars can be as large as 2 times the solar mass.
; DENSITY-DEPENDENT MODEL
; QUASI-PARTICLE MODEL
; GLUON PLASMA
Peng, C,Peng GX,Peng, GX,et al. Magnetized strange quark matter in the equivparticle model with both confinement and perturbative interactions[J]. NUCLEAR SCIENCE AND TECHNIQUES,2016,27(4).
Peng, C,彭光雄,Peng, GX,Xia, CJ,Xu, JF,&Zhang, SP.(2016).Magnetized strange quark matter in the equivparticle model with both confinement and perturbative interactions.NUCLEAR SCIENCE AND TECHNIQUES,27(4).
Peng, C,et al."Magnetized strange quark matter in the equivparticle model with both confinement and perturbative interactions".NUCLEAR SCIENCE AND TECHNIQUES 27.4(2016).