Institut Fresnel, CNRS, Aix-Marseille Université, Ecole Centrale Marseille, Campus de St Jérôme, 13013 Marseille, France.
Nat Commun. 2012;3:1171. doi: 10.1038/ncomms2167.
Magnetodielectric small spheres present unusual electromagnetic scattering features, theoretically predicted a few decades ago. However, achieving such behaviour has remained elusive, due to the non-magnetic character of natural optical materials or the difficulty in obtaining low-loss highly permeable magnetic materials in the gigahertz regime. Here we present unambiguous experimental evidence that a single low-loss dielectric subwavelength sphere of moderate refractive index (n=4 like some semiconductors at near-infrared) radiates fields identical to those from equal amplitude crossed electric and magnetic dipoles, and indistinguishable from those of ideal magnetodielectric spheres. The measured scattering radiation patterns and degree of linear polarization (3-9 GHz/33-100 mm range) show that, by appropriately tuning the a/λ ratio, zero-backward ('Huygens' source) or almost zero-forward ('Huygens' reflector) radiated power can be obtained. These Kerker scattering conditions only depend on a/λ. Our results open new technological challenges from nano- and micro-photonics to science and engineering of antennas, metamaterials and electromagnetic devices.
磁电介质小球呈现出异常的电磁散射特性,这一现象早在几十年前就已被理论预测到。然而,由于天然光学材料不具有磁性,或者难以在千兆赫兹范围内获得低损耗高磁导率的磁性材料,因此实现这种行为一直具有挑战性。在这里,我们给出了明确的实验证据,证明一个低损耗介电亚波长中等折射率(n=4,类似于近红外的一些半导体)球体的辐射场与相等幅度的正交电偶极子和磁偶极子的辐射场相同,并且与理想的磁电介质球体的辐射场无法区分。所测量的散射辐射模式和线性偏振度(3-9 GHz/33-100 mm 范围)表明,通过适当调整 a/λ 比值,可以获得零后向(“惠更斯”源)或几乎零前向(“惠更斯”反射器)辐射功率。这些 Kerker 散射条件仅取决于 a/λ。我们的研究结果为从纳米光子学到天线、超材料和电磁器件的科学和工程领域带来了新的技术挑战。