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Tuning the magnetic properties in MPS3 (M = Mn, Fe, and Ni) by proximity-induced Dzyaloshinskii Moriya interactions 邻域诱导Dzyaloshinskii Moriya相互作用对MPS3 (M = Mn, Fe和Ni)磁性能的调节
Pub Date : 2023-07-25 DOI: arxiv-2307.13400
Suvodeep Paul, Devesh Negi, Saswata Talukdar, Saheb Karak, Shalini Badola, Bommareddy Poojitha, Manasi Mandal, Sourav Marik, R. P. Singh, Nashra Pistawala, Luminita Harnagea, Aksa Thomas, Ajay Soni, Subhro Bhattacharjee, Surajit Saha
Tailoring the quantum many-body interactions in layered materials throughappropriate heterostructure engineering can result in emergent properties thatare absent in the constituent materials thus promising potential futureapplications. In this article, we have demonstrated controlling the otherwiserobust magnetic properties of transition metal phosphorus trisulphides(Mn/Fe/NiPS3) in their heterostructures with Weyl semimetallic MoTe2 which canbe attributed to the Dzyaloshinskii Moriya (DM) interactions at the interfaceof the two different layered materials. While the DM interaction is known toscale with the strength of the spin-orbit coupling (SOC), we also demonstratehere that the effect of DM interaction strongly varies with the spinorientation/dimensionality of the magnetic layer and the low-energy electronicdensity of state of the spin-orbit coupled layer. The observations are furthersupported by a series of experiments on heterostructures with a variety ofsubstrates/underlayers hosting variable SOC and electronic density of states.
通过适当的异质结构工程来剪裁层状材料中的量子多体相互作用可以产生组成材料中不存在的新特性,从而有潜在的未来应用前景。在本文中,我们证明了用Weyl半金属MoTe2控制过渡金属三硫化磷(Mn/Fe/NiPS3)异质结构中的磁性能,这可归因于两种不同层状材料界面上的Dzyaloshinskii Moriya (DM)相互作用。虽然已知DM相互作用与自旋轨道耦合(SOC)的强度成比例,但我们也在这里证明了DM相互作用的影响与磁层的自旋取向/维数和自旋轨道耦合层的低能电子态密度密切相关。这些观察结果得到了一系列异质结构实验的进一步支持,这些异质结构具有各种衬底/衬底承载可变SOC和电子态密度。
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引用次数: 0
Thermal Casimir interactions in multi-particle systems: scattering channel approach 多粒子系统中的热卡西米尔相互作用:散射通道方法
Pub Date : 2023-07-20 DOI: arxiv-2307.10570
Yang Li, Kimball A. Milton, Iver Brevik
Multi-particle thermal Casimir interactions are investigated, mostly in termsof the Casimir entropy, from the point of view based on multiple-scatteringprocesses. The geometry of the scattering path is depicted in detail, and thecontributions from different types of channels, namely the transverse,longitudinal and mixing channels, are demonstrated. The geometry of the pathcan strongly influence the weight of each channel in the path. Negativity andnonmonotonicity are commonly seen in the multi-particle Casimir entropy, thesources of which are diverse, including the geometry of the path, the types ofpolarization mixing, the polarizability of each particle, etc. Thermalcontributions from multi-particle scatterings can be significant in the system,while the zero-temperature multi-particle scattering effects are insignificant.Limiting behaviors from a multi-particle configuration to a continuum arebriefly explored.
从基于多重散射过程的角度出发,主要从卡西米尔熵的角度研究了多粒子热卡西米尔相互作用。详细描述了散射路径的几何形状,并展示了不同类型的通道,即横向通道,纵向通道和混合通道的贡献。路径的几何形状会强烈地影响路径中每个通道的权重。多粒子卡西米尔熵的负性和非单调性是常见的,其来源是多种多样的,包括路径的几何形状、极化混合的类型、每个粒子的极化率等。多粒子散射的热贡献在体系中是显著的,而零温度多粒子散射效应不显著。简要探讨了从多粒子结构到连续体的极限行为。
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引用次数: 0
Investigation of the rotational spectrum of CD$_3$OD and an astronomical search toward IRAS 16293$-$2422 CD$_3$OD旋转光谱的研究及对IRAS 16293$-$2422的天文搜索
Pub Date : 2023-07-15 DOI: arxiv-2307.07801
V. V. Ilyushin, H. S. P. Müller, J. K. Jørgensen, S. Bauerecker, C. Maul, R. Porohovoi, E. A. Alekseev, O. Dorovskaya, F. Lewen, S. Schlemmer, R. M. Lees
Solar-type prestellar cores and protostars display large amounts ofdeuterated organic molecules. Recent findings on CHD$_2$OH and CD$_3$OH towardIRAS 16293-2422 suggest that even fully deuterated methanol, CD$_3$OD, may bedetectable as well. However, searches for CD$_3$OD are hampered in particularby the lack of intensity information from a spectroscopic model. The objectiveof the present investigation is to develop a spectroscopic model of CD$_3$OD inlow-lying torsional states that is sufficiently accurate to facilitate searchesfor this isotopolog in space. We carried out a new measurement campaign forCD$_3$OD involving two spectroscopic laboratories that covers the 34 GHz-1.1THz range. A torsion-rotation Hamiltonian model based on the rho-axis methodwas employed for our analysis. Our resulting model describes the ground andfirst excited torsional states of CD$_3$OD well up to quantum numbers $J leq51$ and $K_a leq 23$. We derived a line list for radio-astronomicalobservations from this model that is accurate up to at least 1.1 THz and shouldbe sufficient for all types of radio-astronomical searches for this methanolisotopolog. This line list was used to search for CD$_3$OD in data from theProtostellar Interferometric Line Survey of IRAS 16293$-$2422 obtained with theAtacama Large Millimeter/submillimeter Array. While we found several emissionfeatures that can be attributed largely to CD$_3$OD, their number is still notsufficiently high enough to establish a clear detection. Nevertheless, theestimate of 2$times 10^{15}$ cm$^{-2}$ derived for the CD$_3$OD column densitymay be viewed as an upper limit that can be compared to column densities ofCD$_3$OH, CH$_3$OD, and CH$_3$OH. The comparison indicates that the CD$_3$ODcolumn density toward IRAS 16293-2422 is in line with the enhanced D/H ratiosobserved for multiply deuterated complex organic molecules.
类太阳的恒星前核和原恒星显示出大量氘化有机分子。最近对diras 16293-2422的CHD $_2$ OH和CD $_3$ OH的研究表明,即使是完全氘化的甲醇CD $_3$ OD也可以检测到。然而,对CD $_3$ OD的搜索受到阻碍,特别是缺乏来自光谱模型的强度信息。本研究的目的是建立一个CD $_3$ OD在低洼扭转状态的光谱模型,该模型足够精确,以促进在空间中寻找这种同位素。我们对cd $_3$ OD进行了新的测量活动,涉及两个光谱实验室,覆盖34 GHz-1.1THz范围。我们的分析采用了基于ro轴方法的扭转-旋转哈密顿模型。我们得到的模型描述了CD的基态和第一激发扭转态$_3$ OD,量子数达到$J leq51$和$K_a leq 23$。我们从该模型中导出了射电天文观测的线表,其精度至少达到1.1太赫兹,并且应该足以用于所有类型的射电天文搜索。利用该线表对利用theAtacama大型毫米波/亚毫米波阵列获得的IRAS 16293 $-$ 2422原恒星干涉线测量数据进行CD $_3$ OD搜索。虽然我们发现了几个主要归因于CD $_3$ OD的排放特征,但它们的数量仍然不够高,不足以建立明确的检测。然而,CD $_3$ OD的柱密度估计为2 $times 10^{15}$ cm $^{-2}$,可以看作是与CD $_3$ OH、CH $_3$ OD和CH $_3$ OH的柱密度相比较的上限。比较表明,对IRAS 16293-2422的CD $_3$ od柱密度与多重氘化复合有机分子的D/H比增强一致。
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引用次数: 0
Modeling laser pulses as $δ$-kicks: reevaluating the impulsive limit in molecular rotational dynamics 将激光脉冲建模为$δ$-kicks:重新评估分子旋转动力学中的脉冲极限
Pub Date : 2023-07-14 DOI: arxiv-2307.07256
Volker Karle, Mikhail Lemeshko
The impulsive limit (the "sudden approximation") has been widely employed todescribe the interaction between molecules and short, far-off-resonant laserpulses. This approximation assumes that the timescale of the laser--moleculeinteraction is significantly shorter than the internal rotational period of themolecule, resulting in the rotational motion being instantaneously "frozen"during the interaction. This simplified description of laser-moleculeinteraction is incorporated in various theoretical models predicting rotationaldynamics of molecules driven by short laser pulses. In this theoretical work,we develop an effective theory for ultrashort laser pulses by examining thefull time-evolution operator and solving the time-dependent Schr"odingerequation at the operator level. Our findings reveal a critical angularmomentum, $l_mathrm{crit}$, at which the impulsive limit breaks down. In otherwords, the validity of the sudden approximation depends not only on the pulseduration, but also on its intensity, since the latter determines how manyangular momentum states are populated. We explore both ultrashort multi-cycle(Gaussian) pulses and the somewhat less studied half-cycle pulses, whichproduce distinct effective potentials. We discuss the limitations of theimpulsive limit and propose a new method that rescales the effective matrixelements, enabling an improved and more accurate description of laser-moleculeinteractions.
脉冲极限(“突然逼近”)已被广泛用于描述分子与短而远的共振激光脉冲之间的相互作用。这个近似假设激光-分子相互作用的时间尺度明显短于分子的内部旋转周期,导致旋转运动在相互作用期间瞬间“冻结”。这种激光-分子相互作用的简化描述被纳入各种理论模型,预测由短激光脉冲驱动的分子的旋转动力学。在这项理论工作中,我们通过检查全时间演化算子和在算子水平上求解时变Schr odinger方程,建立了一个有效的超短激光脉冲理论。我们的发现揭示了一个临界角动量,$l_ mathm {crit}$,在这个角动量处脉冲极限被打破。换句话说,突然逼近的有效性不仅取决于脉冲持续时间,还取决于其强度,因为后者决定了多少个角动量态被填充。我们研究了超短多周期(高斯)脉冲和研究较少的半周期脉冲,它们产生不同的有效电位。我们讨论了脉冲极限的局限性,并提出了一种重新缩放有效矩阵元素的新方法,使激光分子相互作用的描述得到了改进和更准确的描述。
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引用次数: 0
Substrate-Selective Adhesion of Metal Nanoparticles to Graphene Devices 金属纳米颗粒与石墨烯器件的衬底选择性粘附
Pub Date : 2023-07-12 DOI: arxiv-2307.06407
Patrick J. Edwards, Sean Stuart, James T. Farmer, Ran Shi, Run Long, Oleg V. Prezhdo, Vitaly V. Kresin
Nanostructured electronic devices, such as those based on graphene, aretypically grown on top of the insulator SiO2. Their exposure to a flux of smallsize-selected silver nanoparticles has revealed remarkably selective adhesion:the graphene channel can be made fully metallized while the insulatingsubstrate remains coverage-free. This conspicuous contrast derives from the lowbinding energy between the metal nanoparticles and a contaminant-freepassivated silica surface. In addition to providing physical insight intonanoparticle adhesion, this effect may be of value in applications involvingdeposition of metallic layers on device working surfaces: it eliminates theneed for masking the insulating region and the associated extensive andpotentially deleterious pre- and postprocessing.
纳米结构的电子器件,比如基于石墨烯的器件,通常生长在绝缘体SiO2上。它们暴露在小尺寸选定的银纳米颗粒的通量下,显示出显著的选择性粘附:石墨烯通道可以完全金属化,而绝缘衬底保持无覆盖。这种明显的对比源于金属纳米颗粒和无污染钝化二氧化硅表面之间的低结合能。除了提供对颗粒粘附的物理洞察之外,这种效应在涉及器件工作表面金属层沉积的应用中可能具有价值:它消除了屏蔽绝缘区域以及相关的广泛且潜在有害的预处理和后处理的需要。
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引用次数: 0
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arXiv - PHYS - Atomic and Molecular Clusters
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