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引用次数: 0
摘要
本文对作者在研究拓扑宇宙弦短距离真空相互作用过程中取得的最新成果进行了扩展概述,同时考虑到了宇宙弦的横向尺寸 a 和量子化场的质量 m。我们考虑了具有最小耦合的大质量实值标量场的情况。结果表明,在弦间距离明显大于康普顿长度(lc=1/m)的情况下,卡西米尔效应呈指数式减弱。另一方面,在距离小于 lc 但远大于典型弦宽时,场-质量的影响变得微不足道。在这种情况下,大质量场对卡西米尔能量的部分贡献与无质量场的贡献同阶。在这些距离上,弦的横向尺寸也是微不足道的。然而,在与弦半径相同数量级的弦间距离上,粗弦的真空相互作用能量可能会大大超过单位长度质量相同的两根无限细弦的真空相互作用能量。
Vacuum Interaction of Topological Strings at Short Distances
The paper provides an extended overview of recent results obtained by the authors in the process of studying the vacuum interaction of topological cosmic strings at short distances, taking into account their transverse size a and the mass m of the quantized field. We consider the case of a massive real-valued scalar field with minimal coupling. It is shown that at the interstring distances significantly larger than the Compton length, lc=1/m, the Casimir effect is damped exponentially. On the other hand, at distances smaller than lc but much larger than the typical string width, the field-mass influence becomes insignificant. In this case, the partial contribution of a massive field to the Casimir energy is of the same order as the contribution of a massless one. At these distances, the string’s transverse size is insignificant also. However, at the interstring distances of the same order as a string radius, the energy of the vacuum interaction of thick strings may significantly surpass the one for two infinitely thin strings with the same mass per unit length.