Department of Physics and Astronomy, University of Utah, Salt Lake City, USA.
Sci Rep. 2014 Sep 24;4:6456. doi: 10.1038/srep06456.
Optical antennas can be used to manipulate the direction and polarization of radiation from an emitter. Usually, these metallic nanostructures utilize localized plasmon resonances to generate highly directional and strongly polarized emission, which is determined predominantly by the antenna geometry alone, and is thus not easily tuned. Here we show experimentally that the emission polarization can be manipulated using a simple, nonresonant scanning probe consisting of the sharp metallic tip of an atomic force microscope; finite element simulations reveal that the emission simultaneously becomes highly directional. Together, the measurements and simulations demonstrate that interference between light emitted directly into the far field with that elastically scattered from the tip apex in the near field is responsible for this control over polarization and directionality. Due to the relatively weak emitter-tip coupling, the tip must be positioned very precisely near the emitter, but this weak coupling also leads to highly tunable emission properties with a similar degree of polarization and directionality compared to resonant antennas.
光学天线可用于操纵发射器辐射的方向和偏振。通常,这些金属纳米结构利用局域等离子体共振来产生高度定向和强偏振的发射,这主要由天线几何形状决定,因此不容易调节。在这里,我们通过一个简单的非共振扫描探针实验证明了发射偏振可以通过原子力显微镜的尖锐金属尖端来控制;有限元模拟表明,发射同时变得高度定向。测量和模拟结果表明,远场中直接发射的光与近场中从尖端弹性散射的光之间的干涉是导致这种对偏振和方向性控制的原因。由于发射器与尖端的耦合相对较弱,因此必须非常精确地将尖端定位在发射器附近,但这种弱耦合也导致发射特性具有高度可调性,与共振天线相比具有类似程度的偏振和方向性。