Mavromatos Nick E, Papavassiliou Joannis
1Department of Theoretical Physics and IFIC, University of Valencia - CSIC, 46100 Valencia, Spain.
2Theoretical Particle Physics and Cosmology Group, Department of Physics, King's College London, Strand, London, WC2R 2LS UK.
Eur Phys J C Part Fields. 2018;78(1):68. doi: 10.1140/epjc/s10052-018-5542-5. Epub 2018 Jan 24.
It is well known that certain special classes of self-gravitating point-like defects, such as global (non gauged) monopoles, give rise to non-asymptotically flat space-times characterized by solid angle deficits, whose size depends on the details of the underlying microscopic models. The scattering of electrically neutral particles on such space-times is described by amplitudes that exhibit resonant behaviour when thescattering and deficit angles coincide. This, in turn, leads to ring-like structures where the cross sections are formally divergent ("singular lensing"). In this work, we revisit this particular phenomenon, with the twofold purpose of placing it in a contemporary and more general context, in view of renewed interest in the theory and general phenomenology of such defects, and, more importantly, of addressing certain subtleties that appear in the particular computation that leads to the aforementioned effect. In particular, by adopting a specific regularization procedure for the formally infinite Legendre series encountered, we manage to ensure the recovery of the Minkowski space-time, and thus the disappearance of the lensing phenomenon, in the no-defect limit, and the validity of the optical theorem for the elastic total cross section. In addition, the singular nature of the phenomenon is confirmed by means of an alternative calculation, which, unlike the original approach, makes no use of the generating function of the Legendre polynomials, but rather exploits the asymptotic properties of the Fresnel integrals.
众所周知,某些特殊类别的自引力点状缺陷,如整体(非规范)单极子,会产生以立体角亏缺为特征的非渐近平直时空,其大小取决于基础微观模型的细节。电中性粒子在此类时空上的散射由振幅描述,当散射角与亏缺角重合时,振幅会表现出共振行为。这进而导致出现环形结构,其截面形式上发散(“奇异透镜效应”)。在这项工作中,我们重新审视这一特殊现象,有两个目的:鉴于对这类缺陷的理论和一般现象学重新产生兴趣,将其置于当代更一般的背景下;更重要的是,解决在导致上述效应的特定计算中出现的某些微妙问题。特别是,通过对遇到的形式上无穷的勒让德级数采用特定的正则化程序,我们设法确保在无缺陷极限下恢复闵可夫斯基时空,从而使透镜效应消失,并确保弹性总截面的光学定理的有效性。此外,通过一种替代计算证实了该现象的奇异性质,与原始方法不同,这种计算不使用勒让德多项式的生成函数,而是利用菲涅耳积分的渐近性质。