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Toroidal phase topologies within paraxial laser beams 准轴向激光束内的环形相位拓扑结构
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-24 DOI: 10.1038/s42005-024-01782-8
Jinzhan Zhong, Houan Teng, Qiwen Zhan
Control of topologies in structured light fields with multi-degrees of freedom integrates fundamental optical physics and topological invariance. Beyond the simple phase vortex, three-dimensional (3D) topological singularities and related nonsingular textures have recently gained significant interest. Here, we experimentally demonstrate the creation of a family of toroidal phase topologies within paraxial laser beams. By employing single two-dimensional (2D) phase control, we generate propagating 3D topological textures, effectively embodying the topological configuration of a four-dimensional (4D) parameter space. The resulting light fields exhibit amplitude isosurfaces of toroidal vortices and hopfionic phase textures, both controlled by topological charges. The ability to prepare scalar phase textures of light offers new insights into the high-dimensional control of complex structured textures and may find significant applications in light-matter interactions, optical manipulation, and optical information encoding. Exploring non-trivial topologies and related properties has long been a fascinating and challenging task in mathematics and physics. The authors experimentally demonstrate the realization of optical toroidal vortices and hopfionic phase textures within paraxial continuous wave laser beams, which may provide new insight for topologically structured light fields.
在具有多自由度的结构光场中控制拓扑结构融合了基础光学物理和拓扑不变性。除了简单的相位涡旋,三维(3D)拓扑奇异性和相关的非奇异纹理最近也引起了人们的极大兴趣。在这里,我们通过实验演示了在准轴向激光束中产生环状相位拓扑的过程。通过采用单一的二维(2D)相位控制,我们产生了传播的三维拓扑纹理,有效地体现了四维(4D)参数空间的拓扑配置。由此产生的光场表现出环状涡旋的振幅等值面和跳菲奥尼相纹理,两者都由拓扑电荷控制。制备光的标量相纹理的能力为复杂结构纹理的高维控制提供了新的见解,并可能在光物质相互作用、光学操纵和光学信息编码中找到重要应用。长期以来,探索非三维拓扑结构和相关特性一直是数学和物理学中一项引人入胜且极具挑战性的任务。作者通过实验演示了在准轴向连续波激光束中实现光学环形涡旋和跳菲奥尼相纹理,这可能会为拓扑结构光场提供新的见解。
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引用次数: 0
Gravitational lensing reveals cool gas within 10-20 kpc around a quiescent galaxy 引力透镜揭示了静止星系周围 10-20 kpc 范围内的冷气体
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-24 DOI: 10.1038/s42005-024-01778-4
Tania M. Barone, Glenn G. Kacprzak, James W. Nightingale, Nikole M. Nielsen, Karl Glazebrook, Kim-Vy H. Tran, Tucker Jones, Hasti Nateghi, Keerthi Vasan Gopala Chandrasekaran, Nandini Sahu, Themiya Nanayakkara, Hannah Skobe, Jesse van de Sande, Sebastian Lopez, Geraint F. Lewis
While quiescent galaxies have comparable amounts of cool gas in their outer circumgalactic medium (CGM) compared to star-forming galaxies, they have significantly less interstellar gas. However, open questions remain on the processes causing galaxies to stop forming stars and stay quiescent. Theories suggest dynamical interactions with the hot corona prevent cool gas from reaching the galaxy, therefore predicting the inner regions of quiescent galaxy CGMs are devoid of cool gas. However, there is a lack of understanding of the inner regions of CGMs due to the lack of spatial information in quasar-sightline methods. We present integral-field spectroscopy probing 10–20 kpc (2.4–4.8 Re) around a massive quiescent galaxy using a gravitationally lensed star-forming galaxy. We detect absorption from Magnesium (MgII) implying large amounts of cool atomic gas (108.4–109.3 M⊙ with T~104 Kelvin), in comparable amounts to star-forming galaxies. Lens modeling of Hubble imaging also reveals a diffuse asymmetric component of significant mass consistent with the spatial extent of the MgII absorption, and offset from the galaxy light profile. This study demonstrates the power of galaxy-scale gravitational lenses to not only probe the gas around galaxies, but to also independently probe the mass of the CGM due to it’s gravitational effect. Quiescent galaxies have similar amount of cool gas to star forming galaxies, yet why galaxies stop forming stars remains an open question. The authors investigate why passive galaxies remain quiescent using a gravitationally lensed background galaxy to probe the faint, diffuse cool gas around a massive quiescent galaxy, and use lensing configuration to constrain the total mass and geometry of this gas reservoir.
与恒星形成星系相比,静止星系外围星系介质(CGM)中的冷气体数量相当,但它们的星际气体数量要少得多。然而,关于导致星系停止形成恒星并保持静止状态的过程,仍然存在一些未解之谜。理论认为,与热日冕的动力学相互作用阻止了冷气体进入星系,因此预测静止星系CGM的内部区域没有冷气体。然而,由于类星体视线方法缺乏空间信息,人们对CGM的内部区域缺乏了解。我们利用一个引力透镜状恒星形成星系,对一个大质量静止星系周围 10-20 kpc(2.4-4.8 Re)的区域进行了积分场光谱探测。我们探测到了镁(MgII)的吸收,这意味着存在大量的冷原子气体(108.4-109.3 M⊙,T~104开尔文),其数量与恒星形成星系相当。对哈勃成像的透镜建模还揭示了一个弥漫的不对称成分,其质量很大,与 MgII 吸收的空间范围一致,并偏离了星系的光剖面。这项研究展示了星系尺度引力透镜的威力,它不仅可以探测星系周围的气体,还可以独立探测由于引力效应而产生的CGM的质量。静止星系拥有与恒星形成星系相似数量的冷气体,然而星系为什么停止形成恒星仍然是一个未解之谜。作者利用一个引力透镜背景星系来探测大质量静止星系周围微弱、弥漫的冷气体,并利用透镜配置来约束这个气体库的总质量和几何形状,从而研究了被动星系保持静止状态的原因。
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引用次数: 0
Engineering ideal helical topological networks in stanene via Zn decoration 通过锌装饰在链烯中设计理想的螺旋拓扑网络
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-22 DOI: 10.1038/s42005-024-01764-w
Jennifer Coulter, Mark R. Hirsbrunner, Oleg Dubinkin, Taylor L. Hughes, Boris Kozinsky
The xene family of topological insulators plays a key role in many proposals for topological electronic, spintronic, and valleytronic devices. These proposals rely on applying local perturbations, including electric fields and proximity magnetism, to induce topological phase transitions in xenes. However, these techniques lack control over the geometry of interfaces between topological regions, a critical aspect of engineering topological devices. We propose adatom decoration as a method for engineering atomically precise topological edge modes in xenes. Our first-principles calculations show that decorating stanene with Zn adatoms exclusively on one of two sublattices induces a topological phase transition from the quantum spin Hall (QSH) to quantum valley Hall (QVH) phase and confirm the existence of spin-valley polarized edge modes propagating at QSH/QVH interfaces. We conclude by discussing technological applications of these edge modes that are enabled by the atomic precision afforded by recent advances in adatom manipulation technology. The authors propose sublattice-selective decoration by Zn adatoms as a method to engineer precise topological edge modes in xenes. First-principles calculations on Zn decorated stanene reveal a quantum spin Hall (QSH) to quantum valley Hall (QVH) transition and spin-valley polarized modes propagating at the QSH/QVH interface.
烯系拓扑绝缘体在拓扑电子、自旋电子和谷电子器件的许多方案中发挥着关键作用。这些建议依赖于应用局部扰动(包括电场和邻近磁性)来诱导烯的拓扑相变。然而,这些技术缺乏对拓扑区域之间界面几何形状的控制,而这正是拓扑器件工程的一个关键方面。我们提出用金刚体装饰作为一种方法,在二甲苯中设计原子精确的拓扑边缘模式。我们的第一性原理计算表明,在两个亚晶格中的一个亚晶格上用锌金刚原子装饰芒硝,会诱发从量子自旋霍尔(QSH)到量子谷霍尔(QVH)相的拓扑相变,并证实在 QSH/QVH 界面传播的自旋谷极化边缘模式的存在。最后,我们讨论了这些边缘模式的技术应用,这些技术应用得益于金刚原子操纵技术的最新进展所带来的原子精度。作者提出用 Zn 金刚原子进行亚晶格选择性装饰,作为一种在二甲苯中设计精确拓扑边缘模式的方法。对锌装饰茚的第一性原理计算揭示了量子自旋霍尔(QSH)到量子谷霍尔(QVH)的转变,以及在 QSH/QVH 界面传播的自旋谷极化模式。
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引用次数: 0
Anisotropic virtual gain and large tuning of particles’ scattering by complex-frequency excitations 各向异性虚拟增益和复频激励对粒子散射的大幅调谐
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-21 DOI: 10.1038/s42005-024-01772-w
Grigorios P. Zouros, Iridanos Loulas, Evangelos Almpanis, Alex Krasnok, Kosmas L. Tsakmakidis
Active tuning of the scattering of particles and metasurfaces is a highly sought-after property for a host of electromagnetic and photonic applications, but it normally requires challenging-to-control tunable (reconfigurable) or active (gain) media. Here, we introduce the concepts of anisotropic virtual gain and oblique Kerker effect, where a completely lossy anisotropic medium behaves exactly as its anisotropic gain counterpart upon excitation by a synthetic complex-frequency wave. The strategy allows one to largely tune the magnitude and angle of a particle’s scattering simply by changing the shape (envelope) of the incoming radiation, rather than by an involved medium-tuning mechanism. The so-attained anisotropic virtual gain enables directional super-scattering at an oblique direction with fine-management of the scattering angle. Our study is based on analytical techniques that allow multipolar decomposition of the scattered field in agreement with full-wave simulations, and lays the foundations for a light management method. The authors show how the use of suitable time-domain pulses, characterized by a complex frequency, can turn anisotropic losses to anisotropic virtual gain in small particles. These excitations can largely tune the scattering off particles without requiring any other tuning mechanism.
主动调整粒子和元表面的散射是大量电磁和光子应用所渴求的特性,但通常需要具有挑战性的可调(可重构)或主动(增益)介质来控制。在这里,我们引入了各向异性虚拟增益和斜凯尔克效应的概念,即在合成复频波的激励下,完全损耗的各向异性介质表现与其各向异性增益介质完全相同。这种策略使人们只需改变传入辐射的形状(包络线),就能在很大程度上调整粒子散射的幅度和角度,而无需采用介质调整机制。由此获得的各向异性虚拟增益可以实现斜方向的定向超散射,并对散射角进行精细管理。我们的研究基于分析技术,可对散射场进行多极分解,与全波模拟一致,为光管理方法奠定了基础。作者展示了如何使用以复杂频率为特征的适当时域脉冲,将各向异性损失转化为小颗粒中的各向异性虚拟增益。这些激励可以在很大程度上调整粒子的散射,而不需要任何其他调整机制。
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引用次数: 0
Control-enhanced non-Markovian quantum metrology 控制增强型非马尔可夫量子计量学
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-21 DOI: 10.1038/s42005-024-01758-8
Xiaodong Yang, Xinyue Long, Ran Liu, Kai Tang, Yue Zhai, Xinfang Nie, Tao Xin, Jun Li, Dawei Lu
Quantum metrology promises unprecedented precision of parameter estimation, but it is often vulnerable to noise. While significant efforts have been devoted to improving the metrology performance in Markovian environments, practical control schemes specifically designed for non-Markovian noises are much less investigated. Here, we propose two control-enhanced quantum metrology schemes that are suitable for tackling general non-Markovian noises described by noise channels or noise spectra. We conduct experiments to verify the efficacy of these schemes on a nuclear magnetic resonance system. The experimental results involving multiqubit probes show that the parameter estimation precision can be greatly improved, significantly surpassing the standard quantum limit, with our schemes. At present, non-Markovian noises are widely encountered on diverse quantum devices, the proposed schemes are relevant for realistic metrology applications on these platforms. Quantum metrology, a powerful paradigm for surpassing classical measurement precision, has been extensively studied for Markovian noise, while most practical physical processes obey non-Markovian dynamics. In this paper, the authors propose control-enhanced quantum metrology schemes to counteract non-Markovian noise and experimentally verify their efficacy.
量子计量学有望实现前所未有的参数估计精度,但它往往容易受到噪声的影响。虽然人们已经为提高马尔可夫环境下的计量性能付出了巨大努力,但专门针对非马尔可夫噪声设计的实用控制方案却鲜有研究。在这里,我们提出了两种控制增强型量子计量方案,它们适用于处理由噪声通道或噪声频谱描述的一般非马尔可夫噪声。我们在核磁共振系统上进行了实验,以验证这些方案的有效性。涉及多量子比特探针的实验结果表明,采用我们的方案可以大大提高参数估计精度,显著超越标准量子极限。目前,非马尔可夫噪声广泛存在于各种量子设备中,所提出的方案适用于这些平台上的实际计量应用。量子计量学是超越经典测量精度的强大范例,针对马尔可夫噪声进行了广泛研究,而大多数实际物理过程都服从非马尔可夫动力学。在本文中,作者提出了控制增强型量子计量方案,以抵消非马尔可夫噪声,并通过实验验证了其功效。
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引用次数: 0
Ionization by XFEL radiation produces distinct structure in liquid water XFEL 辐射电离产生液态水的独特结构
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-20 DOI: 10.1038/s42005-024-01768-6
Michal Stransky, Thomas J. Lane, Alexander Gorel, Sébastien Boutet, Ilme Schlichting, Adrian P. Mancuso, Zoltan Jurek, Beata Ziaja
In the warm dense matter (WDM) regime, where condensed, gas, and plasma phases coexist, matter frequently exhibits unusual properties that cannot be described by contemporary theory. Experiments reporting phenomena in WDM are therefore of interest to advance our physical understanding of this regime, which is found in dwarf stars, giant planets, and fusion ignition experiments. Using 7.1 keV X-ray free electron laser radiation (nominally 5×105 J/cm2), we produced and probed transient WDM in liquid water. Wide-angle X-ray scattering (WAXS) from the probe reveals a new ~9 Å structure that forms within 75 fs. By 100 fs, the WAXS peak corresponding to this new structure is of comparable magnitude to the ambient water peak, which is attenuated. Simulations suggest that the experiment probes a superposition of two regimes. In the first, fluences expected at the focus severely ionize the water, which becomes effectively transparent to the probe. In the second, out-of-focus pump radiation produces O1+ and O2+ ions, which rearrange due to Coulombic repulsion over 10 s of fs. Our simulations account for a decrease in ambient water signal and an increase in low-angle X-ray scattering but not the experimentally observed 9 Å feature, presenting a new challenge for theory. The ionization via high-intensity X-ray irradiation can cause structural rearrangements within the sample. The authors observe a new structure in ionized liquid water emerging within few femtoseconds from the initial ionization, characterized via a peculiar partial order on a length scale much longer than normally found in water.
在凝聚态、气态和等离子态共存的温致密物质(WDM)体系中,物质经常表现出当代理论无法描述的异常特性。因此,报告 WDM 现象的实验对于推进我们对这一机制的物理理解很有意义,矮星、巨行星和核聚变点火实验中都发现了这一机制。利用 7.1 keV X 射线自由电子激光辐射(名义上 5×105 J/cm2),我们在液态水中产生并探测了瞬态 WDM。探针产生的广角 X 射线散射(WAXS)揭示了在 75 fs 内形成的 ~9 Å 新结构。到 100 fs 时,与这种新结构相对应的 WAXS 峰值与环境水峰值的大小相当,而环境水峰值则有所衰减。模拟结果表明,该实验探测了两种状态的叠加。在第一种情况下,焦点处的通量会使水严重电离,从而使水对探针变得透明。在第二种情况下,焦点外的泵辐射产生 O1+ 和 O2+ 离子,由于库仑斥力,这些离子在 10 秒 fs 的时间内重新排列。我们的模拟解释了环境水信号的减少和低角 X 射线散射的增加,但没有解释实验观察到的 9 Å 特征,这对理论提出了新的挑战。通过高强度 X 射线辐照产生的电离可导致样品内部结构重排。作者观察到电离液态水在初始电离后的几飞秒内出现了一种新结构,其特征是在比通常水长得多的长度尺度上出现了一种奇特的偏序。
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引用次数: 0
Nonequilibrium fast-lithiation of Li4Ti5O12 thin film anode for LIBs 用于 LIB 的 Li4Ti5O12 薄膜阳极的非平衡快速锂化
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-17 DOI: 10.1038/s42005-024-01775-7
Yue Chen, Shaohua Zhang, Jiefeng Ye, Xinyi Zheng, Jian-Min Zhang, Nagarathinam Mangayarkarasi, Yubiao Niu, Hongyi Lu, Guiying Zhao, Jianming Tao, Jiaxin Li, Yingbin Lin, Oleg V. Kolosov, Zhigao Huang
Li4Ti5O12 (LTO) is known for its zero-strain characteristic in electrochemical applications, making it a suitable material for fast-charging applications. Here, we systematically studied the quasi-equilibrium and non-equilibrium lithium-ion transportation kinetics in LTO thin-film electrodes, across a range of scales from the crystal lattice to the microstructured electrodes. At the crystal lattice scale, during the non-equilibrium lithiation process, lithium ions are dispersedly embedded into the 16c position, resulting in more 8a → 16c migration compared with the quasi-equilibrium lithiation, and forming numerous fast lithium diffusion channels inside the LTO lattice. At the microstructural electrode scale, optical spectrum characterizations supported the “nano-filaments” lithiation model in polycrystalline LTO thin-film electrodes during the lithiation process. Our results reveal the patterns of lithium migration and distribution within the LTO thin film electrode under the non-equilibrium and quasi-equilibrium lithiation process, offering profound insights into the potential optimization strategies for enhancing the performance of fast-charging thin film batteries. Li4Ti5O12 (LTO) is an ideal battery material for fastcharging applications. The authors examine Li+ transport in LTO thin film electrodes, revealing that nonequilibrium processes result in unique Li+ occupation states that enhance Li+ diffusion. Findings suggests engineering Li+ occupations in LTO crystal lattice can improve battery performance.
Li4Ti5O12(LTO)因其在电化学应用中的零应变特性而闻名,是一种适合快速充电应用的材料。在此,我们系统地研究了 LTO 薄膜电极中从晶格到微结构电极的准平衡和非平衡锂离子传输动力学。在晶格尺度上,在非平衡锂化过程中,锂离子分散嵌入 16c 位置,导致与准平衡锂化相比更多的 8a → 16c 迁移,并在 LTO 晶格内部形成大量快速锂扩散通道。在微结构电极尺度上,光学光谱表征支持多晶 LTO 薄膜电极在锂化过程中的 "纳米纤丝 "锂化模型。我们的研究结果揭示了非平衡态和准平衡态锂化过程中锂在 LTO 薄膜电极中的迁移和分布模式,为提高快速充电薄膜电池性能的潜在优化策略提供了深刻的见解。Li4Ti5O12(LTO)是一种理想的快速充电应用电池材料。作者对 LTO 薄膜电极中的 Li+ 传输进行了研究,发现非平衡过程会导致独特的 Li+ 占位状态,从而增强 Li+ 扩散。研究结果表明,LTO 晶格中的 Li+ 占位工程可以提高电池性能。
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引用次数: 0
Author Correction: Enhancing shift current response via virtual multiband transitions 作者更正:通过虚拟多波段转换增强移位电流响应
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-17 DOI: 10.1038/s42005-024-01771-x
Sihan Chen, Swati Chaudhary, Gil Refael, Cyprian Lewandowski
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引用次数: 0
Polarization-diverse soliton transitions and deterministic switching dynamics in strongly-coupled and self-stabilized microresonator frequency combs 强耦合和自稳定微谐振子频梳中的偏振多样性孤子跃迁和确定性开关动力学
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-17 DOI: 10.1038/s42005-024-01773-9
Wenting Wang, Alwaleed Aldhafeeri, Heng Zhou, Tristan Melton, Xinghe Jiang, Abhinav Kumar Vinod, Mingbin Yu, Guo-Qiang Lo, Dim-Lee Kwong, Chee Wei Wong
Dissipative Kerr soliton microcombs in microresonators have enabled fundamental advances in chip-scale precision metrology, communication, spectroscopy, and parallel signal processing. Here we demonstrate polarization-diverse soliton transitions and deterministic switching dynamics of a self-stabilized microcomb in a strongly-coupled dispersion-managed microresonator driven with a single pump laser. The switching dynamics are induced by the differential thermorefractivity between coupled transverse-magnetic and transverse-electric supermodes during the forward-backward pump detunings. The achieved large soliton existence range and deterministic transitions benefit from the switching dynamics, leading to the cross-polarized soliton microcomb formation when driven in the transverse-magnetic supermode of the single resonator. Secondly, we demonstrate two distinct polarization-diverse soliton formation routes – arising from chaotic or periodically-modulated waveforms via pump power selection. Thirdly, to observe the cross-polarized supermode transition dynamics, we develop a parametric temporal magnifier with picosecond resolution, MHz frame rate and sub-ns temporal windows. We construct picosecond temporal transition portraits in 100-ns recording length of the strongly-coupled solitons, mapping the transitions from multiple soliton molecular states to singlet solitons. This study underpins polarization-diverse soliton microcombs for chip-scale ultrashort pulse generation, supporting applications in frequency and precision metrology, communications, spectroscopy and information processing. Thermal Instability hinders reliable generation of dissipative Kerr solitons in Silicon Nitride microresonators. The authors investigate a regime where polarization-diverse soliton transitions and deterministic dynamics of a self-stabilized microcomb in a dispersion managed microresonator driven with a single pump laser.
微谐振器中的耗散克尔孤子微蜂窝使芯片级精密计量、通信、光谱学和并行信号处理取得了根本性进展。在这里,我们展示了用单泵浦激光器驱动的强耦合色散管理微谐振器中的自稳定微蜂窝的偏振多样性孤子跃迁和确定性开关动力学。开关动力学是由前后泵浦失谐期间耦合横磁超模和横电超模之间的热折射率差引起的。由于开关动力学,实现了较大的孤子存在范围和确定性转换,从而在单谐振器的横磁超模驱动下形成了交叉偏振孤子微蜂窝。其次,我们展示了两种不同的偏振孤子形成途径--通过泵功率选择产生于混沌波形或周期调制波形。第三,为了观测跨偏振超模转变动态,我们开发了一种参数时间放大镜,具有皮秒分辨率、兆赫帧频和亚纳秒时间窗口。我们在强耦合孤子的 100-ns 记录长度内构建了皮秒级的时间转变肖像,映射了从多孤子分子态到单孤子的转变。这项研究为用于芯片级超短脉冲生成的偏振多样性孤子微蜂窝提供了支持,有助于频率和精密计量、通信、光谱学和信息处理等领域的应用。热不稳定性阻碍了氮化硅微谐振器中耗散克尔孤子的可靠产生。作者研究了用单泵浦激光器驱动的分散管理微谐振器中偏振不同的孤子转换和自稳定微蜂巢的确定性动力学机制。
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引用次数: 0
Quantum dual-path interferometry scheme for axion dark matter searches 用于轴心暗物质搜索的量子双路径干涉测量方案
IF 5.4 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Pub Date : 2024-08-16 DOI: 10.1038/s42005-024-01770-y
Qiaoli Yang, Yu Gao, Zhihui Peng
Exploring the mysterious dark matter is a key quest in modern physics. Currently, detecting axions, a hypothetical particle proposed as a primary component of dark matter, remains a significant challenge due to their weakly interacting nature. Here we show at quantum level that in a cavity permeated by a magnetic field, the single axion-photon conversion rate is enhanced by the cavity quality factor and is quantitatively larger than the classical result by π/2. The axion cavity can be considered a quantum device emitting single photons with temporal separations. This differs from the classical picture and reveals a possibility for the axion cavity experiment to handle the signal sensitivity at the quantum level, e.g., a dual path quantum interferometry with cross-power and second-order correlation measurements. This scheme would greatly reduce the signal scanning time and improve the sensitivity of the axion-photon coupling, potentially leading to the direct observation of axions. Axions are the top contenders for explaining the enigmatic dark matter in the Universe. The authors present the inaugural quantum-level validation of a cavity’s resonant boost to the conversion of axions into photons, thus employing a dual-path interferometry method can greatly enhance the signal-to-noise ratio in the experiments, enabling swifter scans and a better detection sensitivity for the evasive axion dark matter.
探索神秘的暗物质是现代物理学的一项重要任务。目前,由于轴子的弱相互作用性质,探测轴子(一种被认为是暗物质主要成分的假想粒子)仍然是一项重大挑战。在这里,我们在量子水平上表明,在一个磁场渗透的空腔中,单轴子-光子转换率会因空腔质量因子而增强,并在数量上比经典结果大π/2。轴子腔可被视为一个发射具有时间间隔的单光子的量子装置。这与经典图景不同,揭示了轴子腔实验在量子水平上处理信号灵敏度的可能性,例如采用交叉功率和二阶相关测量的双路径量子干涉测量法。这种方案将大大缩短信号扫描时间,提高轴子-光子耦合的灵敏度,从而有可能直接观测到轴子。轴子是解释宇宙中神秘暗物质的首要竞争者。作者首次从量子层面验证了空腔共振对轴子转化为光子的促进作用,因此采用双路径干涉测量方法可以大大提高实验的信噪比,从而实现更快的扫描和更高的探测灵敏度,以探测躲避轴子的暗物质。
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引用次数: 0
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Communications Physics
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