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Casimir energy, fermion fractionalization and stability of a Fermi field in an electric potential in (1+1) dimensions

机译:卡西米尔能,费米子分级和费米场在(1 + 1)维电势中​​的稳定性

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In this paper we compute and study the Casimir energy, vacuum polarization and the resulting fermion fractionalization, the phase shifts and the stability of the bound states of a Dirac field, all due to its interaction with an electric potential in (1+1) dimension. We also explore the inter-relation between these effects. All of these effects are different manifestations of one single source, which is the distortion of the fermionic spectrum and appears as spectral deficiencies in the continua and bound states. We compute and display the spatial densities of these deficiencies and those of the bound states, along with their associated energy densities. We find that in both cases the total spatial densities of states with E > 0 and E < 0 are exact mirror images of each other. Therefore these densities for the complete spectrum are unchanged as compared to the free case, and in particular they remain uniform. The densities of states with E < 0 are precisely the vacuum polarization density and the Casimir energy density, respectively. We find that the vacuum polarization is in general noninteger. We then compute and display the energy densities of the spectral deficiencies in the momentum space, and show that levels exiting or entering the continua leave their distinctive marks on these energy densities. We also use the phase shifts to calculate the Casimir energy and obtain the same result as in the direct calculation. In this problem the Casimir energy is always positive and is on the average an increasing function of the depth and width of the potential. It has a cusp whenever an energy level crosses E = 0. These cusps are local maxima in the extreme relativistic limits. Finally we show that the taking the Casimir energy into account, the total energy will be stable under small fluctuations in the parameters of the potential. However only the first two bound states are absolutely stable in the sense that their total energy is smaller than the mass.
机译:在本文中,我们计算和研究了卡西米尔能量,真空极化以及由此产生的费米子分级,狄拉克场的相移和束缚态的稳定性,这都是由于它与(1 + 1)维中的电势相互作用。我们还探讨了这些影响之间的相互关系。所有这些效应都是单一来源的不同表现形式,即铁离子光谱的畸变,并在连续态和束缚态下表现为光谱缺陷。我们计算并显示这些缺陷和束缚态的空间密度,以及它们相关的能量密度。我们发现,在两种情况下,E> 0和E <0的状态的总空间密度都是彼此精确的镜像。因此,与自由情况相比,完整光谱的这些密度没有变化,特别是保持均匀。 E <0的状态密度分别恰好是真空极化密度和卡西米尔能量密度。我们发现真空极化一般是非整数的。然后,我们计算并显示动量空间中光谱缺陷的能量密度,并表明退出或进入连续峰的能级在这些能量密度上留下了与众不同的标记。我们还使用相移来计算卡西米尔能量,并获得与直接计算相同的结果。在这个问题中,卡西米尔能量总是正的,并且平均而言是电势的深度和宽度的增加函数。每当能级超过E = 0时,它就会出现尖峰。这些尖峰是极端相对论极限中的局部最大值。最后,我们表明,考虑到卡西米尔能量,在势能参数的小波动下,总能量将保持稳定。但是,只有前两个结合态在其总能量小于质量的意义上是绝对稳定的。

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