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2011 Conference on Lasers and Electro-Optics Europe and 12th European Quantum Electronics Conference (CLEO EUROPE/EQEC)最新文献

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Permutationally invariant tomography of a four-qubit symmetric Dicke state 四量子位对称Dicke态的排列不变层析成像
C. Schwemmer, G. Tóth, W. Wieczorek, D. Gross, R. Krischek, H. Weinfurter
Multi-partite entangled quantum states play an important role in quantum information processing with applications, for example, in quantum enhanced metrology or quantum communication. Therefore, efficient measurement schemes to fully characterize these states are needed. However, conventional quantum state tomography which reveals all properties of a quantum state suffers from an exponentially increasing measurement effort with the number of qubits.
多部纠缠量子态在量子信息处理中发挥着重要作用,在量子增强计量、量子通信等领域具有广泛的应用。因此,需要有效的测量方案来充分表征这些状态。然而,传统的量子态断层扫描可以揭示量子态的所有特性,随着量子比特的数量,测量工作量呈指数级增长。
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引用次数: 1
Fast absorption recovery and wavelength conversion in 1.5mm AlInGaAs MQW lasers 1.5mm AlInGaAs MQW激光器的快速吸收恢复和波长转换
R. Green, M. Haji, L. Hou, G. Mezősi, R. Dylewicz, T. Kelly
In recent years there has been a high level of interest in the properties of fast semiconductor saturable absorbers operating at λ ∼ 1.5»m. The applications for these include the fabrication of passively modelocked lasers[1] and wavelength conversion of optical data streams through cross-absorption modulation. To enable these effects to be utilised at the highest repetition rates, very fast absorption recovery times are required, in materials that can be conveniently integrated with optical gain elements. Several methods for achieving very short absorption recovery times have been demonstrated such as the inclusion of high densities of crystal defects in the material and the use of intersubband transitions. However, it is not possible to integrate these with gain elements operating at the same wavelength without the use of expensive and technologically demanding epitaxial regrowth processes.
近年来,人们对工作在λ ~ 1.5»m波段的快速半导体可饱和吸收体的特性有了很高的兴趣。这些技术的应用包括制造被动锁模激光器[1]和通过交叉吸收调制实现光数据流的波长转换。为了使这些效果能够以最高的重复率使用,需要在可以方便地与光学增益元件集成的材料中实现非常快的吸收恢复时间。已经证明了几种实现极短吸收恢复时间的方法,例如在材料中包含高密度的晶体缺陷和使用子带间跃迁。然而,如果不使用昂贵且技术要求高的外延再生工艺,就不可能将这些元件与工作在同一波长的增益元件集成在一起。
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引用次数: 0
Ultrafast laser inscription of an integrated multimode-to-single-modes waveguide transition for astrophotonics 天体光子学中集成多模到单模波导跃迁的超快激光刻录
R. Thomson, T. Birks, S. Leon-Saval, A. Kar, J. Bland-Hawthorn
Astrophotonics is the application of photonic principles to astronomical instrumentation, in order to reduce cost, size, weight and complexity while increasing performance. In astrophotonics the “photonic lantern” (PL) [1–4] is a remarkable photonic device which efficiently couples light between a multimode (MM) optical fibre and a set of degenerate single modes (SMs) which are guided by the cores of either individual SM fibres [1–3] or a multicore optical fibre [4]. If the SMs produced by the PL are arranged into a linear array [5], the PL facilitates the efficient collection of light from a telescope using a MM fibre and the low-loss reformatting of this light into a near diffraction limited input (in one axis) for a spectrometer [6].
天体光子学是将光子原理应用于天文仪器,以降低成本、尺寸、重量和复杂性,同时提高性能。在天体光子学中,“光子灯”(PL)[1-4]是一种非凡的光子器件,它可以在多模(MM)光纤和一组简并单模(SMs)之间有效地耦合光,这些简并单模(SMs)由单个SM光纤[1-3]或多芯光纤[4]的核心引导。如果由PL产生的SMs被安排成线性阵列[5],则PL便于使用MM光纤从望远镜有效地收集光,并将该光的低损耗重新格式化为接近衍射限制的输入(在一个轴上),用于光谱仪[6]。
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引用次数: 7
Theoretical study of dispersive wave generation in ar-filled hollow-core PCF above the plasma threshold 等离子体阈值以上充ar空心芯PCF中色散波产生的理论研究
W. Chang, A. Nazarkin, J. Travers, P. Holzer, J. Nold, N. Y. Joly, P. Russell
Hollow-core photonic-crystal fibre (HC-PCF) [1] provides a highly efficient means for investigating light-matter interactions at sustained intensity levels inaccessible to both traditional bulk setups (due to limited interaction lengths) or conventional optical fibres (due to the low damage threshold of glass). Recent experiments have shown that strong UV pulses can be generated, through emission of dispersive radiation, by launching near-IR femtosecond pulses into a gas-filled kagomé-lattice PCF [2]. Phase-matching to the UV can be accounted for through the special dispersion characteristics of the gas-filled HC-PCF [3]. Shorter UV wavelengths require higher energy pulses, causing the intensity to enter the ionisation regime when pulse propagation will be influenced by the presence of free electrons. The transition from the “traditional” regime where the Kerr effect dominates to the plasma regime where ionisation becomes important (novel in the context of photonic crystal fibres) is studied numerically in this work.
空心光子晶体光纤(HC-PCF)[1]提供了一种高效的方法来研究光-物质相互作用的持续强度水平,这是传统的块体装置(由于相互作用长度有限)或传统光纤(由于玻璃的低损伤阈值)无法实现的。最近的实验表明,通过发射色散辐射,将近红外飞秒脉冲发射到充满气体的kagomacom -lattice PCF中,可以产生强紫外脉冲[2]。通过充气HC-PCF的特殊色散特性,可以解释与UV的相位匹配[3]。较短的紫外波长需要较高的能量脉冲,当脉冲传播将受到自由电子存在的影响时,导致强度进入电离状态。从克尔效应占主导地位的“传统”状态到电离变得重要的等离子体状态(在光子晶体光纤的背景下是新颖的)的转变在本工作中进行了数值研究。
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引用次数: 0
Numerical optimisation of a high-energy end-pumped Ho:YLF slab amplifier 高能端泵浦Ho:YLF平板放大器的数值优化
O. Collett, C. Bollig, M. Esser
Single frequency 2µm sources are useful in varied applications including remote sensing, spectroscopy and nonlinear conversion to the mid-infrared. However, to generate high energy pulses from a 2 µm oscillator is challenging, which is typically overcome by implementing a master oscillator power amplifier approach [1]. We have previously demonstrated a single frequency Ho:YLF laser which produced up to 70 mJ per pulse [2] at 2064nm and subsequently developed a 200W Tm:YLF slab laser to be used as pump source for a power amplifier.
单频2 μ m源可用于各种应用,包括遥感,光谱和非线性转换到中红外。然而,从2 μ m振荡器产生高能量脉冲是具有挑战性的,这通常通过实现主振荡器功率放大器方法[1]来克服。我们之前已经展示了单频Ho:YLF激光器,在2064nm处产生高达70 mJ /脉冲[2],随后开发了200W Tm:YLF平板激光器,用作功率放大器的泵浦源。
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引用次数: 0
Coherent optical imaging through opaque layers 通过不透明层的相干光学成像
E. G. van Putten, D. Akbulut, J. Bertolotti, A. Lagendijk, A. Mosk
Scattering of light is usually seen as a nuisance in microscopy. Scattering limits the penetration depth and strongly deteriorates the achievable resolution. However, by gaining active spatial control over the optical wave front it is possible to manipulate the propagation of scattered light even far in the multiple scattering regime.[1–3] It was recently shown that in this way scattered light can even be exploited for perfect optical focussing.[4] These wave front shaping techniques pave the way for new microscopy methods based on strong light scattering.[5–8]
在显微镜中,光的散射通常被看作是一件麻烦事。散射限制了穿透深度,严重降低了可达到的分辨率。然而,通过获得对光波前的主动空间控制,可以在多重散射状态下操纵散射光的传播。[1-3]最近的研究表明,通过这种方式,散射光甚至可以用于完美的光学聚焦。[4]这些波前整形技术为基于强光散射的新显微镜方法铺平了道路。[5-8]
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引用次数: 0
Group-acceleration matching in tapered optical fibers for maximising the power in the blue-edge of a supercontinuum 在超连续体蓝边最大化功率的锥形光纤群加速匹配
S. Sørensen, A. Judge, C. Thomsen, O. Bang
Tapering has been demonstrated as an effective way of pushing the short-wavelength edge of a supercontinuum (SC) into the deep-blue [1–2]. The spectrum of an SC is comprised by a soliton red-edge linked to a dispersive wave (DW) blue-edge through group-velocity matching (GVM) [3]. The edges are formed when a red-shifting soliton catches up with a DW, allowing them to interact through cross-phase modulation (XPM). Tapering utilises this and allows GVM to shorter wavelength. So far the focus has been on moving the spectral edge, only little attention has been devoted to maximising the power in the blue-edge. Here we demonstrate by numerical simulations that the gradient of the taper has a major impact on the power actually available in the blue-edge.
逐渐变细已被证明是将超连续介质(SC)的短波长边缘推进至深蓝的有效方法[1-2]。SC的谱由孤子红边与色散波(DW)蓝边通过群速度匹配(GVM)连接而成[3]。当红移孤子赶上DW时形成边缘,允许它们通过交叉相位调制(XPM)相互作用。锥形利用了这一点,并允许GVM的波长更短。到目前为止,人们的注意力一直集中在移动光谱边缘上,很少有人关注如何最大化蓝边缘的功率。在这里,我们通过数值模拟证明,锥度的梯度对蓝边实际可用的功率有重大影响。
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引用次数: 1
Yb:CaF2 laser at cryogenic temperature 低温下的Yb:CaF2激光器
S. Ricaud, D. Papadopoulos, P. Camy, J. Doualan, R. Moncorgé, A. Courjaud, E. Mottay, P. Georges, F. Druon
Since its first laser operation in 2004 [1], Yb:CaF2 has been one of the most studied and promising crystals in the realm of Yb-doped materials for DPSSL applications [2,3]. In fact, this crystal gathers several interesting advantages for the development of high-power diode-pumped lasers, among which an excellent thermal conductivity of 9.3 W/m/K[4], comparable to YAG, a broad emission band, extending from about 1010 and 1070 nm and a long emission lifetime of 2.3 ms. And, the last but not the least advantage over its competitors concerns the fact that the crystal growth of pure CaF2 is already well mastered and that ultra-high-quality and very large crystals of Yb:CaF2 could be produced in the near future.
自2004年首次激光操作以来[1],Yb:CaF2已成为用于DPSSL应用的掺镱材料领域中研究最多和最有前途的晶体之一[2,3]。事实上,这种晶体对于高功率二极管泵浦激光器的发展具有几个有趣的优点,其中包括9.3 W/m/K的优异导热系数[4],与YAG相当,发射波段宽,从约1010到1070 nm延伸,发射寿命长,为2.3 ms。与竞争对手相比,最后但并非最不重要的优势在于,纯CaF2的晶体生长已经很好地掌握,并且在不久的将来可以生产出超高质量和非常大的Yb:CaF2晶体。
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引用次数: 0
Light turning mirrors for hybrid integration of optical waveguides in SiON technology and CMOS based photo-detectors 光波导与CMOS光电探测器混合集成的转光镜
F. Çivitci, A. Driessen, H. Hoekstra
An efficient connection of integrated optical components and photo-detectors (PDs) is very important to realize small size and high functionality optoelectronic devices. A number of techniques have been reported to provide such a connection. One of these uses a focusing grating coupler on top of a waveguide (WG) to focus the light to the PD above the WG [1]. However, high volume production of such devices is not possible because no mask can be used to define the grating, owing to its relatively small period. Another technique uses a focused ion beam to mill total internal reflection (TIR) mirrors, but this technique is also not suitable for high volume production [2]. The third technique is based on a metal mirror, at which the desired mirror angle is fabricated by using a superficial layer in the wet etching process [3]. The efficiency of the mirrors is very high, but the thermal budget of the fabrication process is low because the melting temperature of metal layer used in the mirror is low.
集成光学元件与光电探测器的高效连接是实现小尺寸、高功能光电器件的重要途径。据报道,有许多技术可以提供这种连接。其中一种是使用波导(WG)顶部的聚焦光栅耦合器将光聚焦到WG上方的PD[1]。然而,这种器件的大批量生产是不可能的,因为由于其相对较小的周期,没有掩模可以用来定义光栅。另一种技术使用聚焦离子束来磨全内反射(TIR)镜,但这种技术也不适合大批量生产[2]。第三种技术是基于金属镜面,在湿法蚀刻工艺中使用表面层来制造所需的镜面角度[3]。反射镜的效率很高,但由于反射镜所用金属层的熔化温度较低,制造过程的热预算较低。
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引用次数: 2
Answering the big questions in astronomy with astrophotonic spectroscopy 用天体光子光谱学解答天文学中的重大问题
J. Allington-Smith
Astrophotonics offers the means to answer some of the most outstanding questions in astronomy by improving the versatility - and therefore the scientific productivity - of highly-multiplexed and precision spectroscopic systems. Together with the increased collecting aperture of the next generation of telescopes and wide-field Adaptive Optics, large, high-precision surveys of faint objects, selected primarily by mass content rather than luminous output, will be possible. Tight control over the instrument characteristics will also permit recovery of the most subtle spectral features. This requires the imaginative use of photonic devices and principles.
天文光子学通过提高多路复用和精密光谱系统的多功能性,从而提高科学生产力,为天文学中一些最突出的问题提供了答案。再加上下一代望远镜的收集孔径增大和宽视场自适应光学,对微弱天体进行大规模、高精度的调查将成为可能,这些调查主要是通过质量含量而不是发光输出来选择的。对仪器特性的严格控制也将允许恢复最细微的光谱特征。这就需要对光子器件和原理进行富有想象力的运用。
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引用次数: 0
期刊
2011 Conference on Lasers and Electro-Optics Europe and 12th European Quantum Electronics Conference (CLEO EUROPE/EQEC)
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