论文标题
在中间密度的强磁夸克物质中缺乏Debye和Meissner筛选
Lack of Debye and Meissner screening in strongly magnetized quark matter at intermediate densities
论文作者
论文摘要
我们研究了在具有强磁场的存在下,在中间的男性巴属密度区域(以化学势$μ$为特征)冷夸克物质的静态响应。我们特别考虑的是,所谓的磁双性手性密度波(MDCDW)相,该相是由粒子孔对形成的不均匀冷凝物实现的。可以表明,在弱耦合方面,MDCDW相比手性对称性制动现象(MC $χ$ sb)在弱耦合方面更稳定,甚至比手性对称阶段预期在足够高的雄性巴马式化学潜能中实现的手性对称相。计算了单循环近似中MDCDW相的光子极化算子的不同成分。我们发现,在MDCDW阶段,在最低的landau级近似中,没有Debye筛选效果。获得的debye长度取决于振幅$ m $和不均匀冷凝物的调制$ b $,如果关系$ |,则仅与零不同。 μ-B | > m $持有。但是,我们发现在感兴趣的地区,这种不平等不满足。因此,在这些条件下没有进行Debye筛查。另一方面,由于颗粒孔冷凝水是电中性的,因此U(1)电磁基不会被基态折断,因此没有Meissner效应。这些结果对于中子星的天体物理学可能会引起人们的关注。
We study the static responses of cold quark matter in the intermediate baryonic density region (characterized by a chemical potential $μ$) in the presence of a strong magnetic field. We consider in particular, the so-called Magnetic Dual Chiral Density Wave (MDCDW) phase, which is materialized by an inhomogeneous condensate formed by a particle-hole pair. It is shown, that the MDCDW phase is more stable in the weak-coupling regime than the one considered in the magnetic catalysis of chiral symmetry braking phenomenon (MC$χ$SB) and even than the chiral symmetric phase that was expected to be realized at sufficiently high baryonic chemical potential. The different components of the photon polarization operator of the MDCDW phase in the one-loop approximation are calculated. We found that in the MDCDW phase there is no Debye screening neither Meissner effect in the lowest-Landau-level approximation. The obtained Debye length depends on the amplitude $m$ and modulation $b$ of the inhomogeneous condensate and it is only different from zero if the relation $| μ-b| > m$ holds. But, we found that in the region of interest this inequality is not satisfied. Thus, no Debye screening takes place under those conditions. On the other hand, since the particle-hole condensate is electrically neutral, the U(1) electromagnetic group is not broken by the ground state and consequently there is no Meissner effect. These results can be of interest for the astrophysics of neutron stars.