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Advances in Raman-based broadband optical refrigeration

机译:基于拉曼的宽带光学制冷进展

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This work reports progress towards demonstrated Raman-based optical refrigeration. Previously [1] we introduced Ramanrefrigeration and its required photonic structures. Building on the previous, the mechanisms and photonic structures aredetailed and simplified proof-of-concept devices described. Three wavelength bands, two illuminated and one dark, areconsidered. The width of each of these bands is predicated upon the magnitude of the Raman shift of the active layer.Optimally, the first illuminated band is approximately one Raman shift (wavelength) in width. This illuminated band iscapped above (at shorter wavelengths) by a dark band. At longer wavelengths a second illuminated band again oneRaman shift in width is reflected by photonic structuring that forbids light propagation. The dark bands provide anexhaust through which up energy (anti-Stokes) shifted light can be emitted thereby carrying away heat. The Photonicstructure prohibits the propagation of a band of long wavelength light thereby both blocking Stoke’s shifted illuminatedband light and reflecting incident light having these wavelengths. The naturally occurring solar spectrum with its light anddark bands caused by atmospheric absorption is a good match to diamond-based Raman refrigeration. Diamond also hasextremely low absorption and large Raman cross-section especially in small grain form. Proof-of-concept devicesemploying simple one-dimensional photonic structures are the focus of present experimental effort. The prospect ofbroadband refrigeration remains a delicate balance requiring limited absorption and increased Raman cross sectionthrough phonon engineering of the Raman active layer.
机译:这项工作报告了表现出基于拉曼的光学制冷进展。以前[1]我们介绍了拉曼制冷及其所需的光子结构。建立上一个,机制和光子结构是描述的详细和简化验证设备。三个波段,两个照明和一个黑暗,是经过考虑的。这些频带中的每一个的宽度都追求有源层的拉曼偏移的大小。最佳地,第一发光频带大约是一个拉曼偏移(波长)的宽度。这个照明的乐队是通过暗频带盖上上面的(以较短的波长)。在较长的波长下再次发光频带宽度的拉曼偏移被禁止光传播的光子结构反射。黑乐队提供了一个可以通过该能量(抗Stokes)移位光的排气,从而携带远离热量。光子结构禁止长波长光带的传播,从而阻挡斯托克的偏移照亮带光并反射具有这些波长的入射光。天然存在的太阳光谱,其光线和由大气吸收引起的暗带是与钻石的拉曼制冷良好的匹配。钻石也有极低吸收和大型拉曼横截面,尤其是小晶粒形式。验证概念设备采用简单的一维光子结构是目前实验努力的焦点。前景宽带制冷仍然是一个精致的平衡,需要有限的吸收和增加的拉曼横截面通过拉曼有源层的声子工程。

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